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Paper Citation Record · LEDGER

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models

As of 4 August 2026, this Paper Citation Record lists 100 of 300 outbound references and 1 inbound Pith citation observation for arXiv:2605.21062.

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

pith.paper-citation-record.v1
2605.21062 v1

Coverage vector

measured 100 of 300 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 101 of 101 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T01:23:53.888749Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

100 of 300 outbound references displayed

  • verified exact71
  • verified fuzzy18
  • unresolved4
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 2c900334-ffcd-41c6-9977-e851751b491d · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA).

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Modules for Experiments in Stellar Astrophysics (MESA)

Reference 1

Resolution
verified exact
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 8d160d81-3161-4cfb-8f25-f5ba4d5ff066 · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars

Reference 2

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verified exact
local_arxiv, observed 2026-05-21T02:13:54.821867Z

Source-reported events for the cited work

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Observation 9f668c6e-0250-4f46-9213-cd4a3138e7b0 · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions

Reference 3

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local_arxiv, observed 2026-05-21T02:13:55.730935Z

Source-reported events for the cited work

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Observation 977b8a8b-d203-4bf4-9964-2e1d4bc3cc86 · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions

Reference 4

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verified exact
local_arxiv, observed 2026-05-21T02:13:55.686340Z

Source-reported events for the cited work

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Observation ad572590-7673-492c-a690-c0c8ded95038 · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation

Reference 5

Resolution
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local_arxiv, observed 2026-05-21T02:13:55.724405Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 3c87c2e5-6b76-44c6-ae7e-0dbb3d63f3d0 · outbound

This paper cites year = 1955, month = jan, volume =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models year = 1955, month = jan, volume =

Reference 6

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doi, observed 2026-05-21T02:13:54.879632Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation d30a4ae4-0b74-4565-9a59-da6dab1016c9 · outbound

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Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 7

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.646461Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 40b94156-e3e0-4143-b924-36b87b7ece25 · outbound

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Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 8

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.737898Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 4cd82783-989b-47e4-8dce-7b1aba84fff2 · outbound

This paper cites Supernova Light Curves Powered by Fallback Accretion.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Supernova Light Curves Powered by Fallback Accretion

Reference 9

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local_arxiv, observed 2026-05-21T02:13:54.862860Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 42b2ea29-0a16-4be3-9609-6fca826ac47f · outbound

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Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 10

Resolution
verified exact
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation b445c36a-8484-440d-8e74-af3212f6f48e · outbound

This paper cites Supernovae from massive stars with extended tenuous envelopes.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Supernovae from massive stars with extended tenuous envelopes

Reference 11

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local_arxiv, observed 2026-05-21T02:13:55.322485Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 1c0a83dd-ac7f-4a67-b8a8-bc17c63d18b5 · outbound

This paper cites The VLT-FLAMES Tarantula Survey X: Evidence for a bimodal distribution of rotational velocities for the single early B-type stars.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models The VLT-FLAMES Tarantula Survey X: Evidence for a bimodal distribution of rotational velocities for the single early B-type stars

Reference 12

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local_arxiv, observed 2026-05-21T02:13:55.164912Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 65d7c025-d4f5-4fa8-8bb5-c37a5e10eee8 · outbound

This paper cites The chemical make-up of the Sun: A 2020 vision.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models The chemical make-up of the Sun: A 2020 vision

Reference 13

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verified exact
local_arxiv, observed 2026-05-21T02:13:55.644692Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation b207f7fb-28f0-467d-acad-3a8e864ee2fd · outbound

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Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 14

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.570287Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 0f74c25c-186c-4131-8d64-80c8b00ffac2 · outbound

This paper cites J., Swenson , F.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models J., Swenson , F

Reference 15

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.499110Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 916419b2-5fdf-4780-ae9e-9b713304ef9d · outbound

This paper cites A., Zimmerman, G.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models A., Zimmerman, G

Reference 16

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doi, observed 2026-05-21T02:13:55.392443Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation e9f8e6cb-f1f1-4f27-a1f0-7be2a10e733f · outbound

This paper cites H., Amthor, A.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models H., Amthor, A

Reference 17

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doi, observed 2026-05-21T02:13:54.985768Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 02846d47-67a0-42d1-9345-ec7aed2a2064 · outbound

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Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 18

Resolution
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raw_fallback, observed 2026-05-21T02:14:25.936213Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 57227ebe-fb9e-40af-ad09-1bf95897604f · outbound

This paper cites Constraining mixing in massive stars in the Small Magellanic Cloud.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Constraining mixing in massive stars in the Small Magellanic Cloud

Reference 19

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verified exact
local_arxiv, observed 2026-05-21T02:13:55.252697Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation cfddc0f2-4b2e-4e11-b33b-3f2a708729e9 · outbound

This paper cites The Binding Energy Parameter for Common Envelope Evolution.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models The Binding Energy Parameter for Common Envelope Evolution

Reference 20

Resolution
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local_arxiv, observed 2026-05-21T02:13:55.557157Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 4ccc905d-f895-42c3-96de-9f759a98099a · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 21

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doi, observed 2026-05-21T02:13:55.487451Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 9ba80d0d-7b33-4ec1-99af-ba1b7afe4f52 · outbound

This paper cites and LeBlanc , F.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models and LeBlanc , F

Reference 22

Resolution
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arxiv_id, observed 2026-05-21T02:13:55.476551Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation e8167aac-1851-4f55-9675-43931b06b24f · outbound

This paper cites Jiang, F.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Jiang, F

Reference 23

Resolution
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arxiv_id, observed 2026-05-21T02:13:55.089274Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation b344dfa6-fd9d-4c91-a55b-157d36002fdc · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 24

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.627069Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 1e3b6a46-e642-4a93-8f01-9e4be21c2485 · outbound

This paper cites Type Ib and IIb supernova progenitors in interacting binary systems.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Type Ib and IIb supernova progenitors in interacting binary systems

Reference 25

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verified exact
local_arxiv, observed 2026-05-21T02:13:54.944713Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation e5d0b9c7-9054-45ba-93ce-50ab227de2f5 · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 26

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verified exact
doi, observed 2026-05-21T02:13:55.178763Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 60ce5f13-e3a0-443a-8a3f-f578d774e2c2 · outbound

This paper cites doi:10.1088/2514-3433/abb6f0 , adsurl =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models doi:10.1088/2514-3433/abb6f0 , adsurl =

Reference 27

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doi, observed 2026-05-21T02:13:55.318919Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 841f03c4-9675-415e-9133-87ba31485f00 · outbound

This paper cites On the Energy Equation and Efficiency Parameter of the Common Envelope Evolution.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models On the Energy Equation and Efficiency Parameter of the Common Envelope Evolution

Reference 28

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local_arxiv, observed 2026-05-21T02:13:54.974190Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 7cc62de6-311c-4c7b-b2db-6828cec3a79f · outbound

This paper cites Common envelope: enthalpy consideration.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Common envelope: enthalpy consideration

Reference 29

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local_arxiv, observed 2026-05-21T02:13:55.351192Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation a87ccedb-d2f4-41ae-bc9b-3bb16aa72ecf · outbound

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Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 30

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doi, observed 2026-05-21T02:13:54.629102Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:f6abe111a74f577b3f232c30da214a2ccfc328d71c9c1df9bd894776d3f36983

Observation 92254104-b096-48b1-9dd0-8b7543f41328 · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 31

Resolution
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doi, observed 2026-05-21T02:13:55.755557Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:56d2cfe23d6b0ce9b8dd22229ba74d55591ba2b66df187c34815ae79fb1a7792

Observation ce44964a-f4eb-4905-88bb-5dea7a9de1f4 · outbound

This paper cites The spectroscopic Hertzsprung-Russell diagram of Galactic massive stars.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models The spectroscopic Hertzsprung-Russell diagram of Galactic massive stars

Reference 32

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.748439Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d65adc40616f64e13698472933b85dfcca68dbb09296d02f708c610b55a1594a

Observation 6359e72d-18cd-41ad-9499-7b8fc617fc3f · outbound

This paper cites Rotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Rotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones

Reference 33

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local_arxiv, observed 2026-05-21T02:13:55.294688Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 0162d6d9-0bc2-42b8-93c6-002a34ec3764 · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 34

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:14:25.932567Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:7ed8efdc6a60ade0277c5f19cebdaf85c032d1ecc3f5cd48078fada5ccfe4a82

Observation 95a8c163-e026-44db-a48b-3482b3ea6e01 · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 35

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:14:25.917987Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:1d4287d811d21bbcfbb86dd6592d4f126b6038d47a8ab355e5c4a943b2817a13

Observation aa8a13e1-da2c-4961-b0cb-7394f697cabe · outbound

This paper cites Mass-loss predictions for O and B stars as a function of metallicity.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Mass-loss predictions for O and B stars as a function of metallicity

Reference 36

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.516469Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b2e00b307c7fdc094c9b66e12139611a45c73582b75b6c3a675522fc1a9b24d6

Observation 4dd66048-e233-4dbc-8fde-e551c83f33cc · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 37

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:14:25.921722Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:3ca94166b73a9373472859868bc5c90b7c6e36abef0a01f91e0ae2a99badbe95

Observation e6e7e9a3-8ed4-4c49-a373-afa596ee11fd · outbound

This paper cites Towards a better understanding of the evolution of Wolf-Rayet stars and Type Ib/Ic supernova progenitors.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Towards a better understanding of the evolution of Wolf-Rayet stars and Type Ib/Ic supernova progenitors

Reference 38

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:54.927969Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:20e0f3ea7328f0932ecceeae2d060a91db3ac7399728ea0f7d9d01653998878f

Observation 2f8be583-5d24-4d74-9db4-0cd88f7254e7 · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 39

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:14:25.924975Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:29a5eae66a6377f96ed55c683987f73e86316f4a553b3ea9c8f9134e186ab81d

Observation 0edb2d96-05ac-454d-a632-c229126a074f · outbound

This paper cites Presupernova Evolution of Rotating Massive Stars I: Numerical Method and Evolution of the Internal Stellar Structure.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Presupernova Evolution of Rotating Massive Stars I: Numerical Method and Evolution of the Internal Stellar Structure

Reference 40

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.365927Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:2910bb624ccc5cd813bf6f64993ef2bd53453bb56008f00d37253e223b2c58fb

Observation 7bf8916c-c2b5-48d0-991d-6b9c81adb55d · outbound

This paper cites Formation of contact in massive close binaries.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Formation of contact in massive close binaries

Reference 41

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.314457Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:5ca7bd82976c178e3a47c9abd47bd88f08dbae71c6b34f7c3e32c30075e99652

Observation 451d4a8a-2018-47bb-922c-442e86de166f · outbound

This paper cites an unresolved cited work.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Unresolved cited work

Reference 42

Resolution
unresolved
raw_fallback, observed 2026-05-21T02:14:25.928924Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:25b72fd8ba9b1895e6b774e08caa15d97b73aeb113dc409a8f9e07425f821b0d

Observation 393b4c97-e53d-4110-a101-1d3e657cc6a7 · outbound

This paper cites year = 1929, month = nov, volume =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models year = 1929, month = nov, volume =

Reference 43

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.367683Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:4fa53759c2e79de494a46e69e197f5ec58a16284e0bdeeed138f7d1eacdf8be6

Observation 3e7e4abf-a6af-41fd-bff9-91e7f87ab7bb · outbound

This paper cites year = 1950, month = jan, volume =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models year = 1950, month = jan, volume =

Reference 44

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.458011Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:207dfcd944b9069cf9d18bf83460bfc053969ca088ae5a3d7fced35f6dc7367d

Observation f8eafd8e-7038-42a3-a5f4-1616d1f83bc8 · outbound

This paper cites 1967, ApJ, 150, 571, doi: 10.1086/149360.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models 1967, ApJ, 150, 571, doi: 10.1086/149360

Reference 45

Resolution
metadata mismatch
doi, observed 2026-05-21T02:13:54.957914Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:34350f9ddd96dcdbcb4c4bed6e9e971a0125a1a31c013029bcd2b8d4901d8ccf

Observation 3a9d3c83-688c-479e-a947-f486b2c55cc0 · outbound

This paper cites a t station \.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models a t station \

Reference 46

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:14:25.906149Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:2165d20d0dc97b9bdc1652350216ab10cbbce46ef2d4c1e7349396ca9e872b23

Observation b4770e48-91b2-46d2-ac5b-be8dc0c5abd0 · outbound

This paper cites year = 1973, month = jan, volume =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models year = 1973, month = jan, volume =

Reference 47

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.415078Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:d9569df34d725f25efb387294ca1628294e945a64bd87e5a232c40309f434614

Observation a81fb51e-ec9d-4fa7-b4ae-dadee1e79c16 · outbound

This paper cites IV - The influence of rotation.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models IV - The influence of rotation

Reference 48

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.049451Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:05966d8ea00470ef59b52897c85b6fb0289995fc1d07ecdc4485d6c05bf32e7e

Observation c1cfc4bb-42ba-48aa-8675-e0d3823d8b9f · outbound

This paper cites Dynamo action by differential rotation in a stably stratified stellar interior.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Dynamo action by differential rotation in a stably stratified stellar interior

Reference 49

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.054571Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:347a4e60dce9d4aa4ca388c206dbe32c8160c7998b37037c56a52333d45f15b6

Observation 6a82e64a-77e4-4879-a4b1-82cc0df691f9 · outbound

This paper cites Comments on Astrophysics and Space Physics , keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Comments on Astrophysics and Space Physics , keywords =

Reference 50

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:14:25.898658Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:5bd573806cbcbcad5fb1faa4dceae47eb1100ea31ca250185ab04fbfaf18ee2d

Observation 48fc0fd2-9b06-4148-a909-b8d2494fdf68 · outbound

This paper cites Stellar Instability and Evolution , year = 1974, editor =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Stellar Instability and Evolution , year = 1974, editor =

Reference 51

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:13:56.964260Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:5fba36356b403e5a91e8c3afa7d120c18b90220330968e9ef65b0b683525f0e5

Observation 75f20bd5-2c9a-4a7e-9535-742ef9ace871 · outbound

This paper cites Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields

Reference 52

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.174978Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:84c0f748639239e984b05b2323efd5c9368fc457c1b7345b60ec839da654a4c3

Observation f53bbc33-fea0-4880-b91e-41c71fab174b · outbound

This paper cites an unresolved cited work.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Unresolved cited work

Reference 53

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.491540Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:b1b2adfdde1dca39d6ca99bffd4ebddde29da0a3cdd44d05f16c814886b23b86

Observation a15fe04c-7ee2-4a03-8ef9-e10d986fa699 · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 54

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.714010Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:aca1e926d46f0bc5466cde636f28c0ad8ad8d616d4d08730dc9775506959a5fd

Observation 0247b418-79b9-4411-86a5-0be267b905d3 · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 55

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:13:56.969185Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:4eabae7fa58cec042807e9f97c83dc723ae34625ce55fb3b511c5ec06c461aa6

Observation 2744c0f8-3bd0-4894-9868-b091403f28c5 · outbound

This paper cites Single star progenitors of long gamma-ray bursts I: Model grids and redshift dependent GRB rate.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Single star progenitors of long gamma-ray bursts I: Model grids and redshift dependent GRB rate

Reference 56

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.280423Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:bbf311dd42ccb3aeaae3fcca186e4c3d92fee7500f18011b5c50bf4f705d1c8a

Observation 123319f1-9e35-446e-92dd-6531819024f4 · outbound

This paper cites The rotation rates of massive stars: the role of binary interaction through tides, mass transfer and mergers.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models The rotation rates of massive stars: the role of binary interaction through tides, mass transfer and mergers

Reference 57

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:54.969511Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:612f0d04506b173688041b1d8c96f3328947e4ea30d0e7f6d03b609e5e77a73f

Observation f11a1b26-6ba6-47b3-a18e-23780060e84a · outbound

This paper cites and LeBlanc , F.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models and LeBlanc , F

Reference 58

Resolution
metadata mismatch
arxiv_id, observed 2026-05-21T02:13:55.696660Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:a0b9338c4d4b72b3960d0f2ffbd129a2d1b0cce15cc2fbb12c3dc34adae37dc5

Observation ba3bea1f-a145-4163-83b0-c6fb8deba3ac · outbound

This paper cites doi:10.1007/978-3-662-55054-0 , adsurl =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models doi:10.1007/978-3-662-55054-0 , adsurl =

Reference 59

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.700260Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:bddd2eb02ff7800896295ce79a078ec02bfb7778946ac3c4fdd42703ca171f0a

Observation f7784ce2-0ab1-43a1-a3de-9fe148002069 · outbound

This paper cites R., Langer, N., Antoniadis, J., et al.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models R., Langer, N., Antoniadis, J., et al

Reference 60

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.539473Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:7f8ef794ade35f87ce551e27488174695053809af17553a335a547a32b84b382

Observation b59eae22-2ab1-4dfe-ad75-ad237027a3f6 · outbound

This paper cites R., M¨ uller, B., Antoniadis, J., et al.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models R., M¨ uller, B., Antoniadis, J., et al

Reference 61

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.613971Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:9df31f48c7429164dec2c12ffb6aa8deebff77eb37282385ed1eae3ec086b78f

Observation 98ab3450-dbbb-4028-be7f-b7c7e410dcb1 · outbound

This paper cites year = 1993, month = aug, volume =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models year = 1993, month = aug, volume =

Reference 62

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:14:25.902405Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:60230524b445ec801d140909953ba420753a3a6ce58a0b7d51bbe422c31629a4

Observation 06ed470a-8b9d-449d-b154-f29b4fd4183e · outbound

This paper cites A., et al., 2011, @doi [ ] 10.1111/j.1365-2966.2011.18706.x , http://adsabs.harvard.edu/abs/2011MNRAS.417.1621D 417.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models A., et al., 2011, @doi [ ] 10.1111/j.1365-2966.2011.18706.x , http://adsabs.harvard.edu/abs/2011MNRAS.417.1621D 417

Reference 63

Resolution
metadata mismatch
arxiv_id, observed 2026-05-21T02:13:55.483378Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:c1635c469f415eb1f060552ac9dc472357d52fa8aa6054d9cad2972ae0b30b30

Observation 544c9b4a-eeaf-49e5-94eb-90adbc5b6e0b · outbound

This paper cites Interacting Binary Stars , year = 1985, editor =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Interacting Binary Stars , year = 1985, editor =

Reference 64

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:14:25.913589Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:cccf2002cb2d394d8d7e5fc41ff0a5610d35980b64fe6690362ece773d207ba0

Observation 2d8730db-3e13-4f6d-8868-21042d78f2fb · outbound

This paper cites S., & Webbink, R.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models S., & Webbink, R

Reference 65

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.634179Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:b864ad33ccdf4082e78ae008b35ae5243c5be82f0f9544cf1aeb3eb6414d5fc6

Observation 98bb468b-564b-4c5b-a1fe-a269c7ecb975 · outbound

This paper cites The spectroscopic Hertzsprung-Russell diagram.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models The spectroscopic Hertzsprung-Russell diagram

Reference 66

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.437260Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:c2325fa176629f448e7cd0feb8a4ff2d2df1c18c550ceda80a403210005e2038

Observation af9ddfa4-9fc8-4822-a859-66fdb965f417 · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 67

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.592616Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:b9a8677685598870407642a2878a83388dfbf6264583996859df40b8ecab46a1

Observation 6108c442-bf27-4690-bc1c-f557561e3443 · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 68

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:13:56.957200Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:a9cf355b6c2d673c652bd9d3ca53b2c07ef947cf3c2faa87447c2a6d51c8bd9c

Observation 51b1bd76-1938-4779-ad53-cbc36fb66405 · outbound

This paper cites A model of anisotropic winds from rotating stars for evolutionary calculations.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models A model of anisotropic winds from rotating stars for evolutionary calculations

Reference 69

Resolution
verified exact
arxiv_id, observed 2026-05-21T02:13:55.588586Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:d7c935f08384b832b835ad475903ece4eaa29b8ffbe1a15289b2df607a375440

Observation fb6b3972-79d6-49a7-932a-7549e22fd75d · outbound

This paper cites Effects of winds on the leftover hydrogen in massive stars following Roche lobe overflow.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Effects of winds on the leftover hydrogen in massive stars following Roche lobe overflow

Reference 70

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.609545Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d376dbc47e05ef276a210f569b44e2ca253e0b58775465c48b23a6dbf140b467

Observation 477bff21-037d-48c3-b859-a8c92b324f38 · outbound

This paper cites Binary progenitor models of type IIb supernovae.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Binary progenitor models of type IIb supernovae

Reference 71

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.565995Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:7c75b6a567c4fbdd58e024842aed9d24598d94213b04955ba581452033efbeb4

Observation 183c4f83-727b-469a-a98d-167474e48c08 · outbound

This paper cites ApJ , author =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models ApJ , author =

Reference 72

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.081371Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:ec2d6b5c1022c0d7ed408494bda85fca7fedfd77738a3bf5ad19569122e586e3

Observation f7400912-70bf-43f6-8bdc-f675785d9222 · outbound

This paper cites an unresolved cited work.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Unresolved cited work

Reference 73

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.120439Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:33d4e0066775d125e47f9682b350acea410fe7c28aa3c08559811d00a54a46a6

Observation e7fa9c4e-a318-4b1c-9589-8e87563c5d3d · outbound

This paper cites Monthly Notices of the Royal Astronomical Society , author =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Monthly Notices of the Royal Astronomical Society , author =

Reference 74

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.010780Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:ac878665c64f35dc84fcee1b25eef7366189e37e64d3a4182914e09cc9cde8a3

Observation 89903ea0-d76e-4439-b6ed-c128db1c1ee3 · outbound

This paper cites Winds from stripped low-mass Helium stars and Wolf-Rayet stars.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Winds from stripped low-mass Helium stars and Wolf-Rayet stars

Reference 75

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.008351Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:9d787d889f623cb9a98ddea49446b7a2f59c28b0b3612898b82d935fcaee0c22

Observation d65fcb9a-0608-4bb3-b5ba-ad06f5940db3 · outbound

This paper cites Pulsations in red supergiants with high L/M ratio -- Implications for the stellar and circumstellar structure of supernova progenitors.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Pulsations in red supergiants with high L/M ratio -- Implications for the stellar and circumstellar structure of supernova progenitors

Reference 76

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.530088Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:798b2c635258de6ea99107bd644ca867b84dfe346fe8e7adc8ce15bdf3ac4516

Observation 5c7f4586-7859-490b-ac01-41b0a0462747 · outbound

This paper cites Implications of massive close binaries for black hole formation and supernovae.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Implications of massive close binaries for black hole formation and supernovae

Reference 77

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.376498Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:a70c93397b3799c292ef31ff75c1e406f49669365b3bb3119e5d8e596e556373

Observation 4780db4b-0398-4c29-ab8b-fa940994e944 · outbound

This paper cites Efficiency of mass transfer in massive close binaries, Tests from double-lined eclipsing binaries in the SMC.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Efficiency of mass transfer in massive close binaries, Tests from double-lined eclipsing binaries in the SMC

Reference 78

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.602792Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ab1b0f002ed5142a10a5f43911e27e317401b17ac4b5e1c2ff001b2e04668679

Observation 7b2737b7-5d5c-46fc-9354-7dfc0e15491a · outbound

This paper cites The massive binary companion star to the progenitor of supernova 1993J.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models The massive binary companion star to the progenitor of supernova 1993J

Reference 79

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.639702Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:2a477c057badd54170707ea38508ceb92c7a68ac0500e431a2b295df9ba37cda

Observation 6edf8bfc-21ca-475d-9804-21070b040ab2 · outbound

This paper cites Structure and Evolution of Close Binary Systems , year = 1976, editor =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Structure and Evolution of Close Binary Systems , year = 1976, editor =

Reference 80

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:14:25.888027Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:c7f93cf3ba9245681926b785ae610b32a1492c1cad1481ce598dc5fce4f4a703

Observation e92429a0-b009-4f8e-a13d-9abe6711250f · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 81

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.040306Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:1b538be5de6f247fba7daecdafe4f216c79f32d7b7bd0853574ec47ea8f82dca

Observation 5570b35e-2bc9-4cd0-af73-0207d847edb9 · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 82

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:14:25.891408Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:ddc9c7b47679f4297f0ca8e5772e2e2cd5aaed4d9a754864f19134640bfe3613

Observation b246e489-16c4-4662-a17d-2dd0a86c0429 · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 83

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:14:25.884026Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:fab482c545478c4b73a7f2fb8d93369e2a322a503d8da9493d30688a72cdac3d

Observation 1c596bc8-b528-40ce-9dc1-54ac98e923df · outbound

This paper cites an unresolved cited work.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Unresolved cited work

Reference 84

Resolution
unresolved
raw_fallback, observed 2026-05-21T02:14:25.880583Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:56961d2a0eda658f61d1b1e0c3ae41d3aa2e9ee0e220e16a2e20d55b013ca59c

Observation 10dec2c8-10ae-4374-8fa8-9516355e0c7c · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 85

Resolution
verified exact
doi, observed 2026-05-21T02:13:54.867437Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:c91b0da9e2a94f92a1c3a7208a89d71f0addd31207edd47a08b64f83de402f2f

Observation 282d7055-6333-4e3a-9036-9f0ec9eb768d · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 86

Resolution
verified exact
doi, observed 2026-05-21T02:13:54.888719Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:92fc9700611388f28a39563a03e6cb8668b17cbf32f0f470e45f5bcf5167e517

Observation 1852e9c6-07ca-4a90-99b2-04e936baf7ab · outbound

This paper cites Metallicity dependence of turbulent pressure and macroturbulence in stellar envelopes.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Metallicity dependence of turbulent pressure and macroturbulence in stellar envelopes

Reference 87

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:54.537538Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:79b0cec567af675a878f28b3eea4fcfa9d53df91934c2fc6231838bb6253c67d

Observation 31b0c4d0-72d8-459b-8d8d-921710e24e31 · outbound

This paper cites an unresolved cited work.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Unresolved cited work

Reference 88

Resolution
unresolved
raw_fallback, observed 2026-05-21T02:14:25.895025Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:516958f1c0047bd71f161e9bedd6335a8fdf670957702f12c974ddb3122b3475

Observation 11de940d-205a-42f6-97a2-21f92c5db007 · outbound

This paper cites an unresolved cited work.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Unresolved cited work

Reference 89

Resolution
unresolved
raw_fallback, observed 2026-05-21T02:14:25.909893Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:3e5933a19e214b08be4f790fc33f0a8040d97fc7f62908791f6c508defd8592b

Observation 252da886-38f7-4c73-bcfc-7abefc539ea6 · outbound

This paper cites year = 1997, month = feb, volume =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models year = 1997, month = feb, volume =

Reference 90

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.746626Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:703d661fed3591f724d3597c030062fe1c3d220b0a34f7b4793580b7faf47025

Observation 0c082528-e8d9-4807-bd4c-dd7f1c0c0c58 · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 91

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.052715Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:6cc085ee09cdcdf18c42efb41b3f2d93a322241d7e87bfc4016508fde4b37cc1

Observation 3b0eab33-e87b-4a4a-b0b9-160b1520d5d9 · outbound

This paper cites 15th European Workshop on White Dwarfs , year = 2007, editor =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models 15th European Workshop on White Dwarfs , year = 2007, editor =

Reference 92

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:14:25.946529Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:e36163001b9137cf09175ef09603c854504fdb8396d43326dd32e5371fe00f1b

Observation 6ba9f264-367c-44c3-babf-23257693e921 · outbound

This paper cites International Conference on Binaries: in celebration of Ron Webbink's 65th Birthday , year = 2010, editor =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models International Conference on Binaries: in celebration of Ron Webbink's 65th Birthday , year = 2010, editor =

Reference 93

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.462226Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:f900a53ba4619c44bb6b782b6428766ac9ef943fd13b0a9915a2630ffdaf4fd4

Observation d8d4e1ec-2610-410f-8f14-ff62e90a0d45 · outbound

This paper cites Gone with the wind: the impact of wind mass transfer on the orbital evolution of AGB binary systems.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Gone with the wind: the impact of wind mass transfer on the orbital evolution of AGB binary systems

Reference 94

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.680647Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:f7a35f7679e7b81293a793fd421e553e38ce6b56e9fc39dcaf62d2b2a1a7f380

Observation 77fd9c0b-03bc-4d8b-bda4-65b6cfeaa752 · outbound

This paper cites Confined Dense Circumstellar Material Surrounding a Regular Type II Supernova: The Unique Flash-Spectroscopy Event of SN 2013fs.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Confined Dense Circumstellar Material Surrounding a Regular Type II Supernova: The Unique Flash-Spectroscopy Event of SN 2013fs

Reference 95

Resolution
metadata mismatch
local_arxiv, observed 2026-05-21T02:13:55.302374Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d5cd31c76e6ff27cf7aa3f78f69015295bba74681d1ca26b42d84672753c4f84

Observation 0251d9db-cba2-444a-8b9c-90f7c1adf8fb · outbound

This paper cites an unresolved cited work.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Unresolved cited work

Reference 96

Resolution
verified exact
doi, observed 2026-05-21T02:13:54.902895Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:ebeddbeb991e7a930d8421797b2c629337a78a383c1ff0539bbffaf605bf1bd4

Observation cb76ade6-7086-4498-81dc-d2552a25a53e · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 97

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:14:25.943140Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:2ea94bbebd65d38871872ba216899a88b8ab26c602949d249b91598f3b905d33

Observation c2a9f0ce-c878-47aa-a0d0-c119506628d8 · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 98

Resolution
verified fuzzy
raw_fallback, observed 2026-05-21T02:14:25.876711Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:fb56f9012df996e7093ed4af9db552ed72e4c98e119a1bd51214e95bb18168aa

Observation f4743a44-fd47-45d4-9d92-0cf47e58f4aa · outbound

This paper cites keywords =.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models keywords =

Reference 99

Resolution
verified exact
doi, observed 2026-05-21T02:13:55.726197Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:6a384082c724632d4bfaae7a67c78c231b4ccf85cf9f5ae4b5d94eb0fdb1bb26

Observation ea420fba-327d-4445-8c8f-d43f823f1877 · outbound

This paper cites A Simple Approach to the Supernova Progenitor-Explosion Connection.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models A Simple Approach to the Supernova Progenitor-Explosion Connection

Reference 100

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.131694Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d4660486d81287822d445d1e2a3301f639328c8eb120a377266329cae4b2761b

Pith citing papers

Observation 222b55c1-2a56-4660-9a7a-be6c0713bcf6 · inbound

Progenitor models of supernovae interacting with their binary companions cites this paper.

Progenitor models of supernovae interacting with their binary companions Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-01T01:23:53.888749Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T01:23:53.888749Z digest=sha256:118be90b453f55ece360961ef98e692b163d692a1fbfda485a17698ff6797588