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Paper Citation Record · LEDGER

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions

As of 9 August 2026, this Paper Citation Record lists 100 of 134 outbound references and 7 inbound Pith citation observations for arXiv:2505.14780.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2505.14780 v2

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measured 100 of 134 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-07T15:35:16.523252Z

measured 107 of 107 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T16:32:31.518161Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-05-21T21:50:41.471614Z

Reference resolution

100 of 134 outbound references displayed

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Outbound references

Observation 0c17e6fd-7336-4e1b-8b23-0d8bab335dd7 · outbound

This paper cites , " * write output.state after.block = add.period write newline.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions , " * write output.state after.block = add.period write newline

Reference 1

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Observation 5858f5ca-8137-4597-8f96-2069d55fac26 · outbound

This paper cites write newline.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions write newline

Reference 2

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source=arxiv_source observed=2026-08-07T15:35:15.241225Z digest=sha256:5efb77914993b75e0abfff30d1a077375bdf8b37fa3e33f041ad69f3d868925c

Observation 592c4dad-edf8-4312-8a39-7cd68535f6ad · outbound

This paper cites 2016, title Astrophysical Implications of the Binary Black-hole Merger GW150914 , The Astrophysical Journal, 818, L22, 10.3847/2041-8205/818/2/L22.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2016, title Astrophysical Implications of the Binary Black-hole Merger GW150914 , The Astrophysical Journal, 818, L22, 10.3847/2041-8205/818/2/L22

Reference 4

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source=arxiv_source observed=2026-08-07T15:35:15.413630Z digest=sha256:cf5db8bbe87142ab711cac64d3e1d0c8e2b057372aec26f638a1fc6fc8018ba7

Observation 00642320-94cf-4542-92e9-fe43000554ae · outbound

This paper cites POSYDON Version 2: Population Synthesis with Detailed Binary-Evolution Simulations across a Cosmological Range of Metallicities.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions POSYDON Version 2: Population Synthesis with Detailed Binary-Evolution Simulations across a Cosmological Range of Metallicities

Reference 5

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source=arxiv_source observed=2026-08-07T15:35:15.513206Z digest=sha256:b16f06538fcf1645ab880525d726d280a564ec5c6d2a4510a99f380f56effd29

Observation 8abcfb94-f39c-4a01-afc8-d2f1c174bb48 · outbound

This paper cites 1971, title Rapidly Rotating Stars.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 1971, title Rapidly Rotating Stars

Reference 6

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source=arxiv_source observed=2026-08-07T15:35:15.554112Z digest=sha256:9c9940503538bb6e1b3a7a1c5a0a298ae2a774ec55f4f3ad3c4113c3e4f86fc8

Observation 985b1a47-37c9-43b8-a0fe-f7a258254d28 · outbound

This paper cites 2020, title Is HR 6819 a Triple System Containing a Black Hole?: An Alternative Explanation, Astronomy & Astrophysics, 641, A43, 10.1051/0004-6361/202038682.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2020, title Is HR 6819 a Triple System Containing a Black Hole?: An Alternative Explanation, Astronomy & Astrophysics, 641, A43, 10.1051/0004-6361/202038682

Reference 7

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Observation ce9a774e-af8f-42c1-a99f-56f695d4a675 · outbound

This paper cites Binarity at Low Metallicity (BLOeM) -- Multiplicity properties of Oe and Be stars.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Binarity at Low Metallicity (BLOeM) -- Multiplicity properties of Oe and Be stars

Reference 8

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source=arxiv_source observed=2026-08-07T15:35:15.711602Z digest=sha256:2bc14edabfcc574d56ffa68c6a8d1efe53ec4a3c3a7ea1cccf9e60433fe3fe4f

Observation 261e10ed-1fd4-407d-a831-640d5fbda7ac · outbound

This paper cites 2011, title Rotating Massive Main-Sequence Stars: I.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2011, title Rotating Massive Main-Sequence Stars: I

Reference 9

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source=arxiv_source observed=2026-08-07T15:35:15.766515Z digest=sha256:e46818440f551596c5b1c86f6fb8e2d8e13683ae3cfbe74d6f0997cb772adcff

Observation 143ec2bd-f166-433d-b5b4-159330daa7a1 · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 10

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source=arxiv_source observed=2026-08-07T15:35:15.873309Z digest=sha256:0162c6aa6166f33143185ba128349bbea3659309f9ba7ec3dbb7dea1a396fd96

Observation c3a944af-7d31-4c71-ac44-4a032be6f6d2 · outbound

This paper cites 2008, title Non- LTE Monte Carlo Radiative Transfer.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2008, title Non- LTE Monte Carlo Radiative Transfer

Reference 11

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source=arxiv_source observed=2026-08-07T15:35:15.919212Z digest=sha256:6e4948d7b6393299e99dc8615cf3ad0068ff3a5f1ed7a26726f33f36128a3164

Observation b57ea1e0-7258-410f-a513-c7869453b464 · outbound

This paper cites 2014, title The Spectroscopic Hertzsprung-Russell Diagram of Galactic Massive Stars, Astronomy & Astrophysics, 570, L13, 10.1051/0004-6361/201425028.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2014, title The Spectroscopic Hertzsprung-Russell Diagram of Galactic Massive Stars, Astronomy & Astrophysics, 570, L13, 10.1051/0004-6361/201425028

Reference 12

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source=arxiv_source observed=2026-08-07T15:35:15.925695Z digest=sha256:a46d9a5cb6410288ef6b1d4ada71db5a5826d7b8db1f98fb42f72b7abaa43e03

Observation f1139c16-0b98-4305-9ac2-a4241f93b62c · outbound

This paper cites 2016, title Mesa Isochrones and Stellar Tracks ( MIST ).

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2016, title Mesa Isochrones and Stellar Tracks ( MIST )

Reference 13

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source=arxiv_source observed=2026-08-07T15:35:15.936840Z digest=sha256:3395a92fa5e0985f23aab8effc897b6e2ce6cb15477420513c0f095f2c68fa3b

Observation 899be368-f2cb-4c92-89ba-53f34ad1a1cf · outbound

This paper cites 2018, title The Remarkable Be + sdOB Binary HD 55606 I : Orbital and Stellar Parameters , The Astrophysical Journal, 865, 76, 10.3847/1538-4357/aad964.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2018, title The Remarkable Be + sdOB Binary HD 55606 I : Orbital and Stellar Parameters , The Astrophysical Journal, 865, 76, 10.3847/1538-4357/aad964

Reference 14

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doi, observed 2026-08-07T15:38:26.729145Z

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Observation fce589f4-c0ed-4c72-8d0f-56dae1f21233 · outbound

This paper cites 2016, title The Dependence of Convective Core Overshooting on Stellar Mass, Astronomy & Astrophysics, 592, A15, 10.1051/0004-6361/201628779.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2016, title The Dependence of Convective Core Overshooting on Stellar Mass, Astronomy & Astrophysics, 592, A15, 10.1051/0004-6361/201628779

Reference 15

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Observation c3ef3d26-8231-499d-b8e5-368cf55be36e · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 16

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Observation cb807295-54c0-4ae9-bdb3-44b20d8543ad · outbound

This paper cites 1994, title Origin and Evolution of Semi-Detached Binaries : Lyrae and SV Centauri ., Astronomy and Astrophysics, 291, 786.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 1994, title Origin and Evolution of Semi-Detached Binaries : Lyrae and SV Centauri ., Astronomy and Astrophysics, 291, 786

Reference 17

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Observation b31edad4-a253-4e48-9d36-f56ae1c068dc · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 18

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Observation 53ef9656-e4ed-4849-a5db-6b86cfc8e572 · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 19

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Observation 29398640-7fc9-49d6-bfd6-538e84be1876 · outbound

This paper cites 2014, title The Incidence of Stellar Mergers and Mass Gainers among Massive Stars , The Astrophysical Journal, 782, 7, 10.1088/0004-637X/782/1/7.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2014, title The Incidence of Stellar Mergers and Mass Gainers among Massive Stars , The Astrophysical Journal, 782, 7, 10.1088/0004-637X/782/1/7

Reference 20

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Observation 6a657b92-b564-438d-93dd-9fb62f4f92e6 · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 21

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Observation cecc202e-e0e1-4195-88ef-a3f8ce7bdc8d · outbound

This paper cites 2010, title Spin Angular Momentum Evolution of the Long-Period Algols , Monthly Notices of the Royal Astronomical Society, 406, 1071, 10.1111/j.1365-2966.2010.16732.x.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2010, title Spin Angular Momentum Evolution of the Long-Period Algols , Monthly Notices of the Royal Astronomical Society, 406, 1071, 10.1111/j.1365-2966.2010.16732.x

Reference 22

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Observation d02b6bc7-6b44-48b9-9452-173b1b19ad2b · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 23

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Observation 14f431f3-8a23-4f10-b627-d3158d5aa890 · outbound

This paper cites 2023, title An Observed Population of Intermediate-Mass Helium Stars That Have Been Stripped in Binaries, Science, 382, 1287, 10.1126/science.ade4970.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2023, title An Observed Population of Intermediate-Mass Helium Stars That Have Been Stripped in Binaries, Science, 382, 1287, 10.1126/science.ade4970

Reference 24

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Observation 5e7189ef-538a-415b-842f-3406b93fa3ae · outbound

This paper cites 2023, title Advances in Optical / Infrared Interferometry , Annual Review of Astronomy and Astrophysics, 61, 237, 10.1146/annurev-astro-121622-045019.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2023, title Advances in Optical / Infrared Interferometry , Annual Review of Astronomy and Astrophysics, 61, 237, 10.1146/annurev-astro-121622-045019

Reference 25

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Observation 895b4436-fc76-43c9-88a2-5479477973cd · outbound

This paper cites 2008, title Evolution towards the Critical Limit and the Origin of Be Stars, Astronomy & Astrophysics, 478, 467, 10.1051/0004-6361:20078095.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2008, title Evolution towards the Critical Limit and the Origin of Be Stars, Astronomy & Astrophysics, 478, 467, 10.1051/0004-6361:20078095

Reference 26

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no resolver link, observed 2026-08-07T15:35:16.038986Z

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Observation f9e60ffc-d7d5-475b-933c-7a4a8a3fc74b · outbound

This paper cites 2022, title NGC 1850 BH1 Is Another Stripped-Star Binary Masquerading as a Black Hole, Monthly Notices of the Royal Astronomical Society: Letters, 511, 24, 10.1093/mnrasl/slab135.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2022, title NGC 1850 BH1 Is Another Stripped-Star Binary Masquerading as a Black Hole, Monthly Notices of the Royal Astronomical Society: Letters, 511, 24, 10.1093/mnrasl/slab135

Reference 27

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source=arxiv_source observed=2026-08-07T15:35:16.045005Z digest=sha256:ea6c382d837f80147c1a7661c26807bda02c59be18bc7177caa4f30a9cfc8d47

Observation 08227b09-4d7a-4169-8d12-15773821d4e1 · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 28

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source=arxiv_source observed=2026-08-07T15:35:16.054401Z digest=sha256:1157a6335bd049d45ab274d1112fa2d3c09f19f55b94e91bcd93349ebdb1c76c

Observation 4c861c72-2b56-4717-97d1-3a64704d4a37 · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 29

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source=arxiv_source observed=2026-08-07T15:35:16.062830Z digest=sha256:412cc684452ce342f80b62f494be792806144a3a594201cc3e908ec2097b8961

Observation f42ddc42-d1e5-4f01-979e-673aa34484c0 · outbound

This paper cites Andrews, Bavera, et al.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Andrews, Bavera, et al

Reference 30

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source=arxiv_source observed=2026-08-07T15:35:16.071838Z digest=sha256:86b74b2d2232be8903cf893d1a6ef06ae770ae84b4cfdb38fffbb5ad3e619af6

Observation 740e56bf-60d8-43e2-9988-7dcde4b93ff5 · outbound

This paper cites 2013, title Populations of Rotating Stars - I.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2013, title Populations of Rotating Stars - I

Reference 31

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no resolver link, observed 2026-08-07T15:35:16.081913Z

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source=arxiv_source observed=2026-08-07T15:35:16.081913Z digest=sha256:eab0ccec59b7519226709f7f3adb2c06701830e20ca5c1a7d468e0f35cd08927

Observation 56b4aa50-12f3-4035-a179-c05ccd8f4d57 · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 32

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no resolver link, observed 2026-08-07T15:35:16.086889Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.086889Z digest=sha256:be16d98442acdc3c9ded7621603d9975bf1e50c2bc9fcd49f5ed4c9c3b7072e2

Observation 6f97784e-891e-4583-a08a-3d7ba80aee44 · outbound

This paper cites 2020, title The H Emission Line Variations of HR 6819, The Astrophysical Journal, 898, L44, 10.3847/2041-8213/aba51c.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2020, title The H Emission Line Variations of HR 6819, The Astrophysical Journal, 898, L44, 10.3847/2041-8213/aba51c

Reference 33

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source=arxiv_source observed=2026-08-07T15:35:16.092000Z digest=sha256:2ce25f872207492d5fb9e6438f129c8dde363d8279f952047820a073868ab061

Observation 5a5d4b38-e9e7-4a02-97e9-fb5410d1a3a8 · outbound

This paper cites 2009, title The Evolution of Runaway Stellar Collision Products, Astronomy & Astrophysics, 497, 255, 10.1051/0004-6361/200810425.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2009, title The Evolution of Runaway Stellar Collision Products, Astronomy & Astrophysics, 497, 255, 10.1051/0004-6361/200810425

Reference 34

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no resolver link, observed 2026-08-07T15:35:16.099966Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.099966Z digest=sha256:508939b083bbe4a8acfc365fb8e95f751575fe5c07736b13d951027649e7e5d8

Observation e33a127a-60ef-409d-9b8c-f21aa1f21533 · outbound

This paper cites 2025, title Scipy/Scipy: SciPy 1.15.1, , Zenodo 10.5281/zenodo.14630489.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2025, title Scipy/Scipy: SciPy 1.15.1, , Zenodo 10.5281/zenodo.14630489

Reference 35

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no resolver link, observed 2026-08-07T15:35:16.106497Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.106497Z digest=sha256:359e9b88c17ba4951450b023a9b38f424109b9693745c11159edf7bc0386f378

Observation f2d97368-28f4-4d75-aebe-9d3e1274aa1f · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 36

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unresolved
no resolver link, observed 2026-08-07T15:35:16.112933Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.112933Z digest=sha256:4633bab38f5161d23715561d2f9ec47560f557c6c344a4d85ee944ea3e09957a

Observation 4dd19ffe-c6d1-45d0-8caf-fee4f7bdbe9b · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 37

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no resolver link, observed 2026-08-07T15:35:16.119779Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.119779Z digest=sha256:dc276a2570450ad926ad750740bad340568c4470225854789ba809125ade9ad5

Observation 8617d349-b46a-4bfa-816a-1387bc581023 · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 38

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unresolved
no resolver link, observed 2026-08-07T15:35:16.128506Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.128506Z digest=sha256:14e1d01d414b2bff74a5b72c935757a93674b5b1f4f669b67e26a8eae48d055c

Observation 306cd390-423d-4028-954a-f9a54a98c4a7 · outbound

This paper cites 2023, title Stellar Properties of Observed Stars Stripped in Binaries in the Magellanic Clouds , The Astrophysical Journal, 959, 125, 10.3847/1538-4357/ace5a3.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2023, title Stellar Properties of Observed Stars Stripped in Binaries in the Magellanic Clouds , The Astrophysical Journal, 959, 125, 10.3847/1538-4357/ace5a3

Reference 39

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unresolved
no resolver link, observed 2026-08-07T15:35:16.136568Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.136568Z digest=sha256:31d223d6e31c8d48e2b6524dc664bb809dd7b95a38cbadec2e0d90b01ddb770f

Observation 9791e0cb-ced6-44e7-9c81-74f7418fa4c7 · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 40

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unresolved
no resolver link, observed 2026-08-07T15:35:16.144061Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.144061Z digest=sha256:f535f183432098907cdab18da8f91c2097b91ffd975daa8485d9f7be7432d25c

Observation c41f02f6-8e51-4564-94e9-f79889e60b0b · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 41

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unresolved
no resolver link, observed 2026-08-07T15:35:16.151635Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.151635Z digest=sha256:054a012f372e8d45e3763d8cbda3550aefc09f6e93783601464ef52249df2ae7

Observation 3dfa3fa8-c77e-460b-837d-7b45517949b1 · outbound

This paper cites 2020, title Array Programming with NumPy , Nature, 585, 357, 10.1038/s41586-020-2649-2.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2020, title Array Programming with NumPy , Nature, 585, 357, 10.1038/s41586-020-2649-2

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.159685Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.159685Z digest=sha256:c8632cde8ef9e2f02ffa568856e85ae88552d45d7a4b164c861047af29b8b911

Observation 1d460614-3a11-4f79-8198-b20065be1f4e · outbound

This paper cites 2021, title Stringent Upper Limit on Be Star Fractions Produced by Binary Interaction, Astronomy & Astrophysics, 653, A144, 10.1051/0004-6361/202141269.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2021, title Stringent Upper Limit on Be Star Fractions Produced by Binary Interaction, Astronomy & Astrophysics, 653, A144, 10.1051/0004-6361/202141269

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.167744Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.167744Z digest=sha256:c601a382f306e1eb2e5dde065113431b2d12c4123f7588abd7fc8fa90f5525b2

Observation 89fc13ad-f185-49b7-adb4-6204a1b60c57 · outbound

This paper cites 2020, title The Single Star Path to Be Stars, Astronomy and Astrophysics, 633, A165, 10.1051/0004-6361/201937018.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2020, title The Single Star Path to Be Stars, Astronomy and Astrophysics, 633, A165, 10.1051/0004-6361/201937018

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.174192Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.174192Z digest=sha256:025f83acb0837458146c1a7e6300216519ee9ec51bff875df44e421f0375823a

Observation 0ca7e25d-e1cc-4b4b-a7e9-ddc964f42cdf · outbound

This paper cites 1963, title Modes of Mass Ejection by Binary Stars and the Effect on Their Orbital Periods ., The Astrophysical Journal, 138, 471, 10.1086/147659.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 1963, title Modes of Mass Ejection by Binary Stars and the Effect on Their Orbital Periods ., The Astrophysical Journal, 138, 471, 10.1086/147659

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.181173Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.181173Z digest=sha256:9359910fb25d54e6f1af70d7b9d0333afd9a885c8d3860c11975606cbfc96a15

Observation d7cc4d89-9a2c-414d-bf9c-cecc6210ff4e · outbound

This paper cites 2007, title Matplotlib: A 2D Graphics Environment, Computing in Science & Engineering, 9, 90, 10.1109/MCSE.2007.55.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2007, title Matplotlib: A 2D Graphics Environment, Computing in Science & Engineering, 9, 90, 10.1109/MCSE.2007.55

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.187248Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.187248Z digest=sha256:a41d5c4e9bfc61e4f16827db53416cd4d6b0337fd2658e3043491b5b39f45fb7

Observation e9e4be06-4d7f-402c-a47e-859683cfa0b5 · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.194239Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.194239Z digest=sha256:1ec2d645f77502e320693f0ee276b0312535aae42e7225fe4d6dabe77b4d31c1

Observation 3dc190a5-521c-49ab-8241-af7c1d0c53dc · outbound

This paper cites 2002, title Evolution of Binary Stars and the Effect of Tides on Binary Populations, Monthly Notices of the Royal Astronomical Society, 329, 897, 10.1046/j.1365-8711.2002.05038.x.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2002, title Evolution of Binary Stars and the Effect of Tides on Binary Populations, Monthly Notices of the Royal Astronomical Society, 329, 897, 10.1046/j.1365-8711.2002.05038.x

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.200706Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.200706Z digest=sha256:6ccb10b91bee53193db6e5d3d32b221ffe01219fad6bf56c9bff5ae8708c1f2b

Observation 8bf47845-0561-4ddc-9daa-701a343da536 · outbound

This paper cites 1981, title Tidal Evolution in Close Binary Systems., Astronomy and Astrophysics, 99, 126.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 1981, title Tidal Evolution in Close Binary Systems., Astronomy and Astrophysics, 99, 126

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.208415Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.208415Z digest=sha256:824927a7fd43abd8486ccaf601fa3843895ddcb647713efbacbe3bae7973d63d

Observation 0ca2a67f-2524-4b7e-9dcd-0d8e4bde68fc · outbound

This paper cites 2006, title Population Nucleosynthesis in Single and Binary Stars - I.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2006, title Population Nucleosynthesis in Single and Binary Stars - I

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.216978Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.216978Z digest=sha256:2e7edf755c3fc2184a117c31f557c273cc424af293162b43246da76822a033e2

Observation 2fac0cbc-e057-4ecd-89c4-9efc47df01e7 · outbound

This paper cites 2009, title Population Synthesis of Binary Carbon-Enhanced Metal-Poor Stars, Astronomy & Astrophysics, 508, 1359, 10.1051/0004-6361/200912827.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2009, title Population Synthesis of Binary Carbon-Enhanced Metal-Poor Stars, Astronomy & Astrophysics, 508, 1359, 10.1051/0004-6361/200912827

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.223342Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.223342Z digest=sha256:6aa6c255482f6a015d0837523c39f1dcb1d0e48a7b00c1c87fa696ad51b97a7a

Observation 75b08411-0afe-4635-b36d-79d4895192ab · outbound

This paper cites 2004, title A New Synthetic Model for Asymptotic Giant Branch Stars, Monthly Notices of the Royal Astronomical Society, 350, 407, 10.1111/j.1365-2966.2004.07446.x.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2004, title A New Synthetic Model for Asymptotic Giant Branch Stars, Monthly Notices of the Royal Astronomical Society, 350, 407, 10.1111/j.1365-2966.2004.07446.x

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.229262Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.229262Z digest=sha256:0147884ab6befe8a59ca2e4903fd73ff752e14d820796127137665ac3b969255

Observation d124caf9-7acf-4e03-bfe6-cbee58080a0c · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.243626Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.243626Z digest=sha256:3b440ca95dc38cd2dd89d2dc97b59c656cafa10a41d17e856ec4813b7c81b4bd

Observation 740bb97d-af17-4b34-80a3-1a647593aa6d · outbound

This paper cites 2024, title Boron Depletion in Galactic Early B-type Stars Reveals Two Different Main Sequence Star Populations, Astronomy & Astrophysics, 690, A135, 10.1051/0004-6361/202450896.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2024, title Boron Depletion in Galactic Early B-type Stars Reveals Two Different Main Sequence Star Populations, Astronomy & Astrophysics, 690, A135, 10.1051/0004-6361/202450896

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.250197Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.250197Z digest=sha256:7171e23158bb6ea8c6af7ad0f90940a5588ed13b595a33d0e31573c2fca690cd

Observation 9c6ab347-bd43-495a-96bc-568f08ffce1d · outbound

This paper cites 1999, title Commissioning FEROS , the New High-Resolution Spectrograph at La-Silla ., The Messenger, 95, 8.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 1999, title Commissioning FEROS , the New High-Resolution Spectrograph at La-Silla ., The Messenger, 95, 8

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.258004Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.258004Z digest=sha256:13d0f4c5c3adaab37f18bef718092baeaf36c10eeb13d4380eb99e5acdefefd7

Observation da5b3377-f057-4a81-a62d-f253fc0982b4 · outbound

This paper cites 1938, title A New Measure of Rank Correlation, Biometrika, 30, 81, 10.1093/biomet/30.1-2.81.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 1938, title A New Measure of Rank Correlation, Biometrika, 30, 81, 10.1093/biomet/30.1-2.81

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.264104Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.264104Z digest=sha256:ee4d67df8bf8887a4dc25dbfd3439d4998489ea8f0097b073c89b2575ff6154b

Observation fbe36a19-51ab-45da-beb9-7c01b9546658 · outbound

This paper cites 1977, title On the Radii of Accreting Main Sequence Stars., Astronomy and Astrophysics, 54, 539.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 1977, title On the Radii of Accreting Main Sequence Stars., Astronomy and Astrophysics, 54, 539

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.272294Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.272294Z digest=sha256:dadfd93f500b67aa4a9cb51616dfc79970db8c1a7e0e940198f6fb859e3735d2

Observation f5c1987b-9a80-4b2b-989c-87b5544c82b6 · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.277755Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.277755Z digest=sha256:4876802fdc0411da72d81b74d97d119897a4c8ed8f9246e8eec27fd715f05060

Observation 9906b4ae-b43c-4dc0-9542-3b2ac9ac2964 · outbound

This paper cites 2022 b , title Interferometric Detections of sdO Companions Orbiting Three Classical Be Stars , The Astrophysical Journal, 926, 213, 10.3847/1538-4357/ac4266.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2022 b , title Interferometric Detections of sdO Companions Orbiting Three Classical Be Stars , The Astrophysical Journal, 926, 213, 10.3847/1538-4357/ac4266

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.285311Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.285311Z digest=sha256:d0227d2015f448f34be3f9dfad1d609ff9f94d09f92f9c392edef4e1814ce2f6

Observation c789b7a1-722a-44a7-a1f0-0c1207a1e716 · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.291136Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.291136Z digest=sha256:e51db9a7b53d83054cbbf0c10a20d9656e4c2fb46403bc2bb9e24ebb80a80eac

Observation b3a4d79a-0d1e-4762-a9a5-262644795702 · outbound

This paper cites 2025, title VLTI / GRAVITY Enables the Determination of the First Dynamical Masses of a Classical Be + Stripped and Bloated Pre-Subdwarf Binary, arXiv, 10.48550/arXiv.2501.04103.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2025, title VLTI / GRAVITY Enables the Determination of the First Dynamical Masses of a Classical Be + Stripped and Bloated Pre-Subdwarf Binary, arXiv, 10.48550/arXiv.2501.04103

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.297353Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.297353Z digest=sha256:5f2f38e35b669e836b1b5d1b476296b1bf1d7c1fac6e0c979e1bb2c2181f5cca

Observation a0d04492-763f-4d4d-942f-fbc47511cda9 · outbound

This paper cites 2009, title A Binary Origin for `blue Stragglers' in Globular Clusters, Nature, 457, 288, 10.1038/nature07635.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2009, title A Binary Origin for `blue Stragglers' in Globular Clusters, Nature, 457, 288, 10.1038/nature07635

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.303017Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.303017Z digest=sha256:7e9b8169c75673b081f0dc76ccf27eb1321f95a66994164091a08ccf1e93994c

Observation 47795a58-6202-4363-b534-c9305c3bde33 · outbound

This paper cites 1990, title A Comparative Study of the Evolution of a Close Binary Using a Standard and an Improved Technique for Computing Mass Transfer., Astronomy and Astrophysics, 236, 385.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 1990, title A Comparative Study of the Evolution of a Close Binary Using a Standard and an Improved Technique for Computing Mass Transfer., Astronomy and Astrophysics, 236, 385

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.309832Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.309832Z digest=sha256:847abde91405f1b36a2757011c97e99eac1e8f6f88bb617e5d2717474d5cedd3

Observation 644a2f32-6fc2-48fc-834b-3e87e76b901f · outbound

This paper cites 2011, title Mass and Angular Momentum Loss via Decretion Disks, Astronomy & Astrophysics, 527, A84, 10.1051/0004-6361/201015951.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2011, title Mass and Angular Momentum Loss via Decretion Disks, Astronomy & Astrophysics, 527, A84, 10.1051/0004-6361/201015951

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.314535Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.314535Z digest=sha256:380f06ae4f8b613917fea370c60c7dd8702503e0ac8d16de80fc32ed0ebacdcb

Observation 626da892-4e2e-41ef-acd4-bc6f2600d6fa · outbound

This paper cites 1985, title Evolution of Massive Stars with Semiconvective Diffusion, Astronomy and Astrophysics, 145, 179.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 1985, title Evolution of Massive Stars with Semiconvective Diffusion, Astronomy and Astrophysics, 145, 179

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.319365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.319365Z digest=sha256:29a528925193945e4a5ec3a1c3acfa81f5378a7ad9dfb12f91640dbe430a07b6

Observation 2054236d-ee41-4c97-b2d8-903e83da53ce · outbound

This paper cites Binary evolution models with rotation.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Binary evolution models with rotation

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.324749Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.324749Z digest=sha256:35677c87bf04d66238d957b42aeca2e44b3abb8c082fdc4fbcfa6a6c680894ac

Observation 7b120291-1150-426f-a358-67643330fc11 · outbound

This paper cites 2020, title The Expansion of Stripped-Envelope Stars: Consequences for Supernovae and Gravitational-Wave Progenitors, Astronomy & Astrophysics, 637, A6, 10.1051/0004-6361/201937300.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2020, title The Expansion of Stripped-Envelope Stars: Consequences for Supernovae and Gravitational-Wave Progenitors, Astronomy & Astrophysics, 637, A6, 10.1051/0004-6361/201937300

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.331020Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.331020Z digest=sha256:76947457532e016d8d3973fcb97594ea4db15d19f1f2165937b81328978001f9

Observation 511d7e58-7f1f-454d-8d2d-064b29dc217a · outbound

This paper cites 2024, title Expansion of Accreting Main-sequence Stars during Rapid Mass Transfer , The Astrophysical Journal, 966, L7, 10.3847/2041-8213/ad3d50.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2024, title Expansion of Accreting Main-sequence Stars during Rapid Mass Transfer , The Astrophysical Journal, 966, L7, 10.3847/2041-8213/ad3d50

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.338997Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.338997Z digest=sha256:9cf0e9ad62c2c70a861605be4bb84cc3a4ab92da5d9fb1c995bafbe782d78f85

Observation 3695a724-77a5-44bc-8392-c3c9bd37f138 · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.344925Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.344925Z digest=sha256:32d9012bdc686c565bd1550da9d30d3d4acb24ee5a78ede3412f26345bfde63b

Observation 72b1b079-bcd5-4046-8f9c-4893f4a18230 · outbound

This paper cites 2021, title The Role of Mass Transfer and Common Envelope Evolution in the Formation of Merging Binary Black Holes, Astronomy & Astrophysics, 650, A107, 10.1051/0004-6361/202039992.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2021, title The Role of Mass Transfer and Common Envelope Evolution in the Formation of Merging Binary Black Holes, Astronomy & Astrophysics, 650, A107, 10.1051/0004-6361/202039992

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.352337Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.352337Z digest=sha256:814afabe175cf3366303eec64279a86a66609187d300722cd942d08d9e5f71af

Observation d3f3be03-c2ca-467f-87d2-cb958a5d538c · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.361544Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.361544Z digest=sha256:13c0c14258851a92d27052fd6b83d1061dbeef05972f298a363c711a74baf25c

Observation c8431519-3ad4-4f1a-920a-8dcfa1284007 · outbound

This paper cites 2013, title On the Accretion Disc and Evolutionary Stage of Lyrae , Monthly Notices of the Royal Astronomical Society, 432, 799, 10.1093/mnras/stt515.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2013, title On the Accretion Disc and Evolutionary Stage of Lyrae , Monthly Notices of the Royal Astronomical Society, 432, 799, 10.1093/mnras/stt515

Reference 72

Resolution
verified exact
doi, observed 2026-08-07T15:35:18.274547Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-08-07T15:35:16.366641Z digest=sha256:0e8af1ba64cba0bab0d606836d6670a5cdd8bd91a80e60e9a03c2f4cb2e68043

Observation 6c4bf3ca-7c17-4d4c-8191-c761e5440793 · outbound

This paper cites 2015, title Spectral and Spatial Imaging of the Be + sdO Binary Persei , Astronomy & Astrophysics, 577, A51, 10.1051/0004-6361/201425141.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2015, title Spectral and Spatial Imaging of the Be + sdO Binary Persei , Astronomy & Astrophysics, 577, A51, 10.1051/0004-6361/201425141

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.371859Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.371859Z digest=sha256:fe3f9d95d435b84ddfc08ab06eb2e78bc333c66526ca48fb1dc5e60a29a3b551

Observation d4866430-5e7d-405a-a745-9189d30366d4 · outbound

This paper cites 2001, title A Complete Survey of Case A Binary Evolution with Comparison to Observed Algol-type Systems , The Astrophysical Journal, 552, 664, 10.1086/320560.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2001, title A Complete Survey of Case A Binary Evolution with Comparison to Observed Algol-type Systems , The Astrophysical Journal, 552, 664, 10.1086/320560

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.376624Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.376624Z digest=sha256:0f4441cc5b7f1bf1bf02a02416443419818530973cd97382c7a9b7917119c479

Observation ef936bd2-c810-4172-a7ab-eea1378df244 · outbound

This paper cites 1977, title Effect of Rapid Mass Accretion onto the Main-Sequence Stars , Publications of the Astronomical Society of Japan, 29, 249.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 1977, title Effect of Rapid Mass Accretion onto the Main-Sequence Stars , Publications of the Astronomical Society of Japan, 29, 249

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.382380Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.382380Z digest=sha256:6004db94a786ef0274b28f6543ea3b10d7b3ca3fa76c3df52210100ffc851507

Observation 50cd172a-570b-4244-aef5-80c05d860e20 · outbound

This paper cites WR + O binaries as probes of the first phase of mass transfer.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions WR + O binaries as probes of the first phase of mass transfer

Reference 76

Resolution
verified exact
local_arxiv, observed 2026-08-07T15:35:18.175477Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-08-07T15:35:16.387867Z digest=sha256:8ece658d77515eb4c91a610ccf6f2cbab6703dc3b484393d5b934f5524761a15

Observation d59a606c-63ca-4827-8beb-1151f7fa92b6 · outbound

This paper cites The Origin and Evolution of Multiple Star Systems.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions The Origin and Evolution of Multiple Star Systems

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.396832Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.396832Z digest=sha256:b222186da116cfcb49d674793bb39261784e71ae4e66173b29a8afa8bbe46b02

Observation 293fabfd-495f-44a5-8a93-1d8be9e5e88d · outbound

This paper cites 1981, title On the Spin-up of the Mass Accreting Component in a Close Binary System, p, 102, 17.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 1981, title On the Spin-up of the Mass Accreting Component in a Close Binary System, p, 102, 17

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.401989Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.401989Z digest=sha256:ac2e5b82b294bfe4515add10a658f8a862bb5a61add64b568c791c39f4f7c53c

Observation 3559f0e4-4298-4101-9651-6508af1ca517 · outbound

This paper cites 1991, title A Polytropic Model of an Accretion Disk, a Boundary Layer, and a Star, The Astrophysical Journal, 370, 597, 10.1086/169846.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 1991, title A Polytropic Model of an Accretion Disk, a Boundary Layer, and a Star, The Astrophysical Journal, 370, 597, 10.1086/169846

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.406766Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.406766Z digest=sha256:16112765b5bfdee7dcba90f66a5c5fc39974966f5842e53837c4235077c9837a

Observation ba214523-19d6-45ba-b378-76e28ed2005f · outbound

This paper cites 2011, title Modules for Experiments in Stellar Astrophysics ( MESA ), The Astrophysical Journal Supplement Series, 192, 3, 10.1088/0067-0049/192/1/3.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2011, title Modules for Experiments in Stellar Astrophysics ( MESA ), The Astrophysical Journal Supplement Series, 192, 3, 10.1088/0067-0049/192/1/3

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.411177Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.411177Z digest=sha256:a5b12a1631ebccc5b309656492ba969df1d7ab853645c248dea1471051f3621e

Observation 260a7379-15f6-4fc8-a5ee-44b7176bf986 · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.415704Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.415704Z digest=sha256:dafad4e95a409c1e46b0dc2140d8e4359c99f9c4df85de8da5e7407ef75e66a3

Observation aae24ff7-b03f-432b-9a9b-1c7c7f6e47ad · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.420364Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.420364Z digest=sha256:40d3e2f78303c22bfece495b91e67fbd1c49cf4c4669961ad34d2d1cec8cb44e

Observation 88eba10e-0dfb-4d31-ad93-2aa99c03289f · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.425891Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.425891Z digest=sha256:2be13ead19d1f96b683b4ae1dcbff4b32e933b96ffa3c074a3c1a9e09db37615

Observation f046bfcd-fe59-4c31-b2ed-e0f42f8f9395 · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.431289Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.431289Z digest=sha256:2bb3466df1b9cbf2e71d7eb5167e03cc356876d39c67d8ec4fc6e4c018b7503d

Observation d17b7e37-7a6d-4a93-8da8-94fc9efc93dc · outbound

This paper cites 2008, title Detection of a Hot Subdwarf Companion to the Be Star FY Canis Majoris , The Astrophysical Journal, 686, 1280, 10.1086/591145.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2008, title Detection of a Hot Subdwarf Companion to the Be Star FY Canis Majoris , The Astrophysical Journal, 686, 1280, 10.1086/591145

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.436546Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.436546Z digest=sha256:62d0eb70f5fd02a9801a410bb8bcd5134311e8212ef9858950a37d837cb6994a

Observation 43685f23-c6c2-4151-b1c3-0f5128066ef2 · outbound

This paper cites 2013, title FAR-ULTRAVIOLET DETECTION OF THE SUSPECTED SUBDWARF COMPANION TO THE Be STAR 59 CYGNI , The Astrophysical Journal, 765, 2, 10.1088/0004-637X/765/1/2.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2013, title FAR-ULTRAVIOLET DETECTION OF THE SUSPECTED SUBDWARF COMPANION TO THE Be STAR 59 CYGNI , The Astrophysical Journal, 765, 2, 10.1088/0004-637X/765/1/2

Reference 86

Resolution
verified exact
doi, observed 2026-08-07T15:35:17.911661Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-08-07T15:35:16.441351Z digest=sha256:9f3fefbbbbe86fef5572ab484049c6c57e36e088b44189cff425b2ac08d35ce6

Observation 7b5c62a6-1cc2-414c-bcf5-58379ab5c473 · outbound

This paper cites 2016, title THE HOT COMPANION AND CIRCUMBINARY DISK OF THE Be STAR HR 2142, The Astrophysical Journal, 828, 47, 10.3847/0004-637X/828/1/47.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2016, title THE HOT COMPANION AND CIRCUMBINARY DISK OF THE Be STAR HR 2142, The Astrophysical Journal, 828, 47, 10.3847/0004-637X/828/1/47

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.447933Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.447933Z digest=sha256:3089909c83beadbff2c77471322187aef06077fd706061183c36a89e4c6c52e8

Observation 79c1ef4d-e526-4c30-9944-764e7cfae8f0 · outbound

This paper cites an unresolved cited work.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Unresolved cited work

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.453765Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.453765Z digest=sha256:dc9bf5759b7b28bf8c17c08dc2d8daa3c437f76200d0bd59b5d54041458684a7

Observation ff31390f-1cf6-4eef-b58a-bbd6e1984c5b · outbound

This paper cites 2005 b , title Which Massive Stars Are Gamma-Ray Burst Progenitors? Astronomy & Astrophysics, 435, 247, 10.1051/0004-6361:20042545.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2005 b , title Which Massive Stars Are Gamma-Ray Burst Progenitors? Astronomy & Astrophysics, 435, 247, 10.1051/0004-6361:20042545

Reference 89

Resolution
verified exact
doi, observed 2026-08-07T15:35:17.822766Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-08-07T15:35:16.460405Z digest=sha256:fed19ac998e09e0be6eb004c6562cd565570a752910c930db472b2fe73127de0

Observation a4fe8c53-6d48-4b1e-8a6b-0b416ede6e8b · outbound

This paper cites 1992, title Presupernova Evolution in Massive Interacting Binaries , The Astrophysical Journal, 391, 246, 10.1086/171341.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 1992, title Presupernova Evolution in Massive Interacting Binaries , The Astrophysical Journal, 391, 246, 10.1086/171341

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.465989Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.465989Z digest=sha256:c18181bfb7d452889b83703663f6d1e3fd9f97f3da8a3752e73cff55bb2d0eae

Observation ed7720ce-110f-486e-8bc5-b5ade9142770 · outbound

This paper cites 2007, in Astronomical Society of the Pacific Conference Series , Vol.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2007, in Astronomical Society of the Pacific Conference Series , Vol

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.471275Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.471275Z digest=sha256:3442d2c50245a4d973db7568ef02eb5f1b2f4ce0b623caeb4fbd831d8f8f4b40

Observation a8629eb3-34c6-4f8b-a373-77ae7d0e0ec8 · outbound

This paper cites 1991, title The Formation of Be Stars through Close Binary Evolution., p, 241, 419.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 1991, title The Formation of Be Stars through Close Binary Evolution., p, 241, 419

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.476848Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.476848Z digest=sha256:6726ccfbaf517317adfbc89dce621848a9c02c488999bfa7f47fbf2a556c8429

Observation a445d365-2cc4-473f-b8c8-9f067ab56124 · outbound

This paper cites 1991, title Does Accretion Cease When a Star Approaches Breakup ? The Astrophysical Journal, 370, 604, 10.1086/169847.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 1991, title Does Accretion Cease When a Star Approaches Breakup ? The Astrophysical Journal, 370, 604, 10.1086/169847

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.481118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.481118Z digest=sha256:9fee41013f4f83cda03dddca1217f0df748bc50fd63349f74626ec0fc56bf7b7

Observation 36320caf-3f24-44d4-8ef4-c10dfbea5b46 · outbound

This paper cites 2003, title Classical Be Stars , Publications of the Astronomical Society of the Pacific, 115, 1153, 10.1086/378307.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2003, title Classical Be Stars , Publications of the Astronomical Society of the Pacific, 115, 1153, 10.1086/378307

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.486679Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.486679Z digest=sha256:a8095530d7e6682fc9c0ff76b65f4a8e0bfd454a70255ea30881f4fd01c31240

Observation afa0349d-f7b9-4b67-9f59-1c300a41079b · outbound

This paper cites 2020, title A Naked-Eye Triple System with a Nonaccreting Black Hole in the Inner Binary, Astronomy & Astrophysics, 637, L3, 10.1051/0004-6361/202038020.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2020, title A Naked-Eye Triple System with a Nonaccreting Black Hole in the Inner Binary, Astronomy & Astrophysics, 637, L3, 10.1051/0004-6361/202038020

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.491252Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.491252Z digest=sha256:2e91b2dcc43b60f40cce1674bacc48d946c395262bdb1a291f38a6af5abd0d44

Observation 5ee6a333-14b6-44ea-93f5-995a79e7d02e · outbound

This paper cites 2013, title Classical Be Stars, The Astronomy and Astrophysics Review, 21, 69, 10.1007/s00159-013-0069-0.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2013, title Classical Be Stars, The Astronomy and Astrophysics Review, 21, 69, 10.1007/s00159-013-0069-0

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.495587Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.495587Z digest=sha256:2bfb35ff62a990a6fd9148507178dc7074ffb239c04a462b07c20cc847efc48d

Observation 9897ea73-dda1-4620-bbe5-49c3528af3fd · outbound

This paper cites 2024, title Classical Be Stars, arXiv, 10.48550/arXiv.2411.06882.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2024, title Classical Be Stars, arXiv, 10.48550/arXiv.2411.06882

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.500080Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.500080Z digest=sha256:e2caf66ab8cca60cc12212cdab2adac97cc1abbf56996b2b836f0a91985452a4

Observation 59374a09-f02e-4e5a-978a-ace6aabf0d45 · outbound

This paper cites 2023, title Bayesian Sampling with BeAtlas , a Grid of Synthetic Be Star Spectra I.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2023, title Bayesian Sampling with BeAtlas , a Grid of Synthetic Be Star Spectra I

Reference 98

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.505322Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.505322Z digest=sha256:ce53dfb41255990ee1c585e0a3e06f192806208dc13606a4a1cded4da07d91da

Observation 150684ba-34cb-4574-93a5-521da0bc0690 · outbound

This paper cites 2012, title Binary Interaction Dominates the Evolution of Massive Stars , Science, 337, 444, 10.1126/science.1223344.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2012, title Binary Interaction Dominates the Evolution of Massive Stars , Science, 337, 444, 10.1126/science.1223344

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.510476Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.510476Z digest=sha256:69bd100c67a579529691d9fb29f8796163cb14db97d29c7c13505456f2f4c10b

Observation 4e57a23c-7639-4a08-863b-a6dbfe7f3ac4 · outbound

This paper cites 2021, title The K2 M67 Study : Precise Mass for a Turnoff Star in the Old Open Cluster M67 , The Astronomical Journal, 161, 59, 10.3847/1538-3881/abca8d.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2021, title The K2 M67 Study : Precise Mass for a Turnoff Star in the Old Open Cluster M67 , The Astronomical Journal, 161, 59, 10.3847/1538-3881/abca8d

Reference 100

Resolution
verified exact
doi, observed 2026-08-07T15:35:17.513916Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-08-07T15:35:16.515861Z digest=sha256:102ece1a9c10579c07159a4092ded9fa6f1881c4a687b79563fc83c863610a12

Observation b31a2126-2860-4e9f-bfbc-ff4226a49762 · outbound

This paper cites 2015, title EVOLUTION OF MASS FUNCTIONS OF COEVAL STARS THROUGH WIND-MASS LOSS AND BINARY INTERACTIONS , The Astrophysical Journal, 805, 20, 10.1088/0004-637X/805/1/20.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions 2015, title EVOLUTION OF MASS FUNCTIONS OF COEVAL STARS THROUGH WIND-MASS LOSS AND BINARY INTERACTIONS , The Astrophysical Journal, 805, 20, 10.1088/0004-637X/805/1/20

Reference 101

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.523252Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.523252Z digest=sha256:e53ce9bdf626f497e82a13a19c8707364bea84734127057cd33eb36a72737887

Pith citing papers

Observation 49a6f2db-0065-4314-a739-7ff3d3729a63 · inbound

A Be Star + He Star Binary as an Indicator of a Binary Mass Transfer Phase cites this paper.

A Be Star + He Star Binary as an Indicator of a Binary Mass Transfer Phase Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-07T11:23:51.739301Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T11:23:51.739301Z digest=sha256:75c6e667d15a40812849abaf3ff594840b632d45ecb9c4834ef3ca59375f00bd

Observation 14785d09-b0d7-4e03-9868-3fc63fb640f4 · inbound

Massive Interacting Binaries Enhance Feedback in Star-Forming Regions cites this paper.

Massive Interacting Binaries Enhance Feedback in Star-Forming Regions Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-06T20:26:51.876251Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T20:26:51.876251Z digest=sha256:a91161ae1d25afe57d1fdd138585762a4243f8fb674caf7a670eb14f3a6c5c81

Observation 4c68e17d-66a9-4ff1-be74-6b5520c38c8c · inbound

Hidden massive eclipsing binaries in red supergiant systems: The hierarchical triple system KQ Puppis and other candidates cites this paper.

Hidden massive eclipsing binaries in red supergiant systems: The hierarchical triple system KQ Puppis and other candidates Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions

Reference 71

Resolution
verified exact
arxiv_id, observed 2026-05-21T21:50:41.473356Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-05-21T21:45:41.836536Z digest=sha256:9425510b0e97a66997fd2184847d9e9eba271ec451802a56a4ef7b6b8ee1a40d

Observation 03030eec-dcc5-4a05-93b2-07a5a83aae5d · inbound

Stable mass transfer in massive binaries leading to merging black holes cites this paper.

Stable mass transfer in massive binaries leading to merging black holes Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions

Reference 136

Resolution
unresolved
no resolver link, observed 2026-08-03T14:34:36.305853Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T14:34:36.305853Z digest=sha256:804b116da24a4b8611cb1955203540caba10a5fa6c1d31b85034418a552767dd

Observation 0d35e841-b49e-4b36-a5f5-d7879eff3c77 · inbound

Toward 3D orbits of wide sdO/B binaries I. Six composite systems spatially resolved with VLTI/GRAVITY cites this paper.

Toward 3D orbits of wide sdO/B binaries I. Six composite systems spatially resolved with VLTI/GRAVITY Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-01T01:39:04.486852Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T01:39:04.486852Z digest=sha256:13e5fc9f2b0a5bed1e9616410801af6d80aadbc53deb628567ed50a2b66a6f25

Observation 1f25c817-b2f0-462d-8b2e-476fdeb179f8 · inbound

A Galactic intermediate-mass stripped star with a Wolf-Rayet-like wind cites this paper.

A Galactic intermediate-mass stripped star with a Wolf-Rayet-like wind Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-08T16:32:31.518161Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T16:32:31.518161Z digest=sha256:0332fe6fea76380bad641e15bf1bd060d5de0fb1f2edf68a3e7bbff2c840e66d

Observation f15de4c5-f4c9-4f90-8495-31260dc6714f · inbound

The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars cites this paper.

The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions

Reference 160

Resolution
unresolved
no resolver link, observed 2026-08-08T13:33:06.757277Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T13:33:06.757277Z digest=sha256:a0d1c1498efba2d5dc29a81e743caf6125be8d5801ced5938d904644bd4afacd