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Paper Citation Record · LEDGER

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants

As of 17 August 2026, this Paper Citation Record lists 98 of 98 outbound references and 0 inbound Pith citation observations for arXiv:2608.11010.

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

pith.paper-citation-record.v1
2608.11010 v2

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measured 98 of 98 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-15T14:18:47.809382Z

measured 98 of 98 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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measured 0 of 1 external citation measurements

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Reference resolution

98 of 98 outbound references displayed

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Outbound references

Observation 47a4d621-f55c-45e4-937d-58f19ac57858 · outbound

This paper cites Post-Asymptotic Giant Branch Evolution of Low- and Intermediate-Mass Stars. Preliminary Results.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Post-Asymptotic Giant Branch Evolution of Low- and Intermediate-Mass Stars. Preliminary Results

Reference 1

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Observation 8b246d1a-9812-4189-a1ef-4271c186e0e0 · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 2

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source=arxiv_source observed=2026-08-15T14:18:43.023549Z digest=sha256:7c8fe33f5967f7ab89b0fa35201bc951f54f446fa4833a01116a60485fc01d8d

Observation 17e60a9f-1a12-4fa1-a7fb-d04d13900d02 · outbound

This paper cites Pulsating white dwarfs: new insights.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Pulsating white dwarfs: new insights

Reference 3

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source=arxiv_source observed=2026-08-15T14:18:43.079089Z digest=sha256:c634512f292483c9ece9f8104fcdc88cfd9064bab9a64b9850698a2804d8b4dc

Observation 95c286c9-a080-4dcd-987f-cad17e6fa4bf · outbound

This paper cites Asteroseismic inferences on GW Vir variable stars in the frame of new PG 1159 evolutionary models.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Asteroseismic inferences on GW Vir variable stars in the frame of new PG 1159 evolutionary models

Reference 4

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source=arxiv_source observed=2026-08-15T14:18:43.085119Z digest=sha256:ef1c145ca6a90cbea2f47f695538cc6cd116b7aa5a4e48a190c63556066c9e91

Observation 814332ec-23f3-4646-a6ad-f0f235a64535 · outbound

This paper cites Rossby numbers and stiffness values inferred from gravity-mode asteroseismology of rotating F- and B-type dwarfs: consequences for mixing, transport, magnetism, and convective penetration.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Rossby numbers and stiffness values inferred from gravity-mode asteroseismology of rotating F- and B-type dwarfs: consequences for mixing, transport, magnetism, and convective penetration

Reference 5

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source=arxiv_source observed=2026-08-15T14:18:43.150604Z digest=sha256:31100c4e1bfa2cc3ca75a5c811095a76e356998d6f308562ca0953f0f4438c7f

Observation 2ca3dd32-13e4-49bb-aadd-b3cc85a7ec75 · outbound

This paper cites K2 photometry and HERMES spectroscopy of the blue supergiant rho Leo: rotational wind modulation and low-frequency waves.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants K2 photometry and HERMES spectroscopy of the blue supergiant rho Leo: rotational wind modulation and low-frequency waves

Reference 6

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source=arxiv_source observed=2026-08-15T14:18:43.189240Z digest=sha256:b18d1b6c9f54b3e7303ca257380ce68f47018d397981ec813d4df2c3d97460bf

Observation 5424279d-2e2c-4f31-b57f-3ba38736f4e8 · outbound

This paper cites Equatorially trapped Rossby waves in radiative stars.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Equatorially trapped Rossby waves in radiative stars

Reference 7

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Observation e8d18e82-a73a-40c3-8a68-de926cd1fe4c · outbound

This paper cites Rossby waves on stellar equatorial beta-planes: uniformly rotating radiative stars.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Rossby waves on stellar equatorial beta-planes: uniformly rotating radiative stars

Reference 8

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Observation 26932db4-c6da-44ac-88bc-c0f53431af3e · outbound

This paper cites Galaxies , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Galaxies , keywords =

Reference 9

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Observation b092e10c-e48c-4581-a627-5e8474a6fdbd · outbound

This paper cites an unresolved cited work.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Unresolved cited work

Reference 10

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Observation dcd66164-27e6-47c5-bcf5-dd649fae1680 · outbound

This paper cites Variability in the CoRoT photometry of three hot O-type stars. HD 46223, HD 46150 and HD 46966.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Variability in the CoRoT photometry of three hot O-type stars. HD 46223, HD 46150 and HD 46966

Reference 11

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Observation 6ff9e8c5-3ea6-4565-a9d0-7af6f7c55b40 · outbound

This paper cites The formation and evolution of hydrogen-deficient post-AGB white dwarfs: the emerging chemical profile and the expectations for the PG1159-DB-DQ evolutionary connection.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants The formation and evolution of hydrogen-deficient post-AGB white dwarfs: the emerging chemical profile and the expectations for the PG1159-DB-DQ evolutionary connection

Reference 12

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Observation 42d782b5-c13c-4971-af3d-de8e41919623 · outbound

This paper cites Low-frequency gravity waves in blue supergiants revealed by high-precision space photometry.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Low-frequency gravity waves in blue supergiants revealed by high-precision space photometry

Reference 13

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Observation 5b8f0c5e-def0-49d1-b064-5927271065fd · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 14

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Observation 5c35cd53-f06a-49ac-bf4d-0835b277f0c5 · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 15

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Observation 7ece4dcf-d72f-4f0a-a7cf-d8f6909b4699 · outbound

This paper cites Variability of Galactic blue supergiants observed with TESS.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Variability of Galactic blue supergiants observed with TESS

Reference 16

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Observation 105ba33a-7908-4744-8f74-cef1629da47a · outbound

This paper cites Confirming the 115.5-day periodicity in the X-ray light curve of ULX NGC 5408 X-1.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Confirming the 115.5-day periodicity in the X-ray light curve of ULX NGC 5408 X-1

Reference 17

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Observation a47ff458-3420-4681-a6e5-112a26ee70c5 · outbound

This paper cites an unresolved cited work.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Unresolved cited work

Reference 18

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Observation f98cd94f-15d1-4fd5-a7c4-d453e96593bb · outbound

This paper cites doi:10.26093/cds/vizier.1350 , adsurl =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants doi:10.26093/cds/vizier.1350 , adsurl =

Reference 19

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Observation cfe1e052-89bc-4ede-bc12-fb1379ee05d1 · outbound

This paper cites TESS photometry of helium-rich hot subdwarfs: r modes in BD+37 442 and BD+37 1977.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants TESS photometry of helium-rich hot subdwarfs: r modes in BD+37 442 and BD+37 1977

Reference 20

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Observation e5dd50b6-d9fb-41b9-adc6-8b1ccd79b337 · outbound

This paper cites Software and Cyberinfrastructure for Astronomy IV , year = 2016, editor =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Software and Cyberinfrastructure for Astronomy IV , year = 2016, editor =

Reference 21

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Observation 45c81b36-516f-48e4-8370-2f11d83508c0 · outbound

This paper cites an unresolved cited work.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Unresolved cited work

Reference 22

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Observation d89a5c86-b569-4d54-a40a-7f49206e85d1 · outbound

This paper cites Stochastic light variations in hot stars from wind instability: Finding photometric signatures and testing against the TESS data.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Stochastic light variations in hot stars from wind instability: Finding photometric signatures and testing against the TESS data

Reference 23

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Observation cc3f814d-9b79-4351-a993-43604f35ba61 · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 24

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Observation 9a63a9b0-b69d-4b3f-9dab-3f9dccb9cf30 · outbound

This paper cites Bright OB stars in the Galaxy.II. Wind variability in O supergiants as traced by H-alpha.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Bright OB stars in the Galaxy.II. Wind variability in O supergiants as traced by H-alpha

Reference 25

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Observation 685e34d7-d275-410e-b303-14776befc87d · outbound

This paper cites an unresolved cited work.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Unresolved cited work

Reference 26

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source=arxiv_source observed=2026-08-15T14:18:44.285850Z digest=sha256:b96a2d72821057e5f9d0a0f55de5030177d2de79025a6249cfa76612e665423d

Observation 823c05e4-1e62-43e6-a79a-3976ef90c525 · outbound

This paper cites The MiMeS survey of Magnetism in Massive Stars: Magnetic properties of the O-type star population.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants The MiMeS survey of Magnetism in Massive Stars: Magnetic properties of the O-type star population

Reference 27

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Observation 6d097726-7e46-4564-b552-d33200ccd0ea · outbound

This paper cites A BRITE view on the massive O-type supergiant V973 Scorpii: Hints towards internal gravity waves or subsurface convection zones.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants A BRITE view on the massive O-type supergiant V973 Scorpii: Hints towards internal gravity waves or subsurface convection zones

Reference 28

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Observation e9ac1d6c-7057-4676-930d-6000208e60e6 · outbound

This paper cites To clump or not to clump The impact of wind inhomogeneities on the optical and NIR spectroscopic analysis of massive OB stars.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants To clump or not to clump The impact of wind inhomogeneities on the optical and NIR spectroscopic analysis of massive OB stars

Reference 29

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Observation f5169082-67b5-44f6-8a4b-39b352ec34fa · outbound

This paper cites Journal of Marine Research , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Journal of Marine Research , keywords =

Reference 30

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Observation 0e1b9e83-6075-4e15-9b33-2b32b28982a8 · outbound

This paper cites Stellar rotation rates in Kepler eccentric (heartbeat) binaries obtained from r-mode signatures.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Stellar rotation rates in Kepler eccentric (heartbeat) binaries obtained from r-mode signatures

Reference 31

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source=arxiv_source observed=2026-08-15T14:18:44.452350Z digest=sha256:f45a509ecbdc0e793358c2681dd09f3ed48f0563fd388af96cddba0d206ac932

Observation 71c2858c-3b3b-450b-b505-6874eb68127a · outbound

This paper cites Theory and evidence of global Rossby waves in upper main-sequence stars: r-mode oscillations in many Kepler stars.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Theory and evidence of global Rossby waves in upper main-sequence stars: r-mode oscillations in many Kepler stars

Reference 32

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Observation 1bdda94e-a9c3-49d4-9c1f-08b6b5c80c78 · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 33

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Observation 44a9d0c8-8293-4433-bd6f-158a36b3e80f · outbound

This paper cites an unresolved cited work.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Unresolved cited work

Reference 34

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source=arxiv_source observed=2026-08-15T14:18:44.567935Z digest=sha256:110752c9c843930c95fb22b56722691106fb7947c2f1009c0b0e2467b934be2f

Observation 016516c3-516c-4a0c-98dc-3a0372bad458 · outbound

This paper cites Low-frequency photospheric and wind variability in the early-B supergiant HD 2905.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Low-frequency photospheric and wind variability in the early-B supergiant HD 2905

Reference 35

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Observation 25e64801-5c1b-426a-be5c-807d5c9b7945 · outbound

This paper cites The IACOB project: III. New observational clues to understand macroturbulent broadening in massive O- and B-type stars.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants The IACOB project: III. New observational clues to understand macroturbulent broadening in massive O- and B-type stars

Reference 36

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source=arxiv_source observed=2026-08-15T14:18:44.699030Z digest=sha256:c9193becae05d70467e862b5184193bb5b1256f33617bcac23e380673dbf90b9

Observation e6c2f596-ae10-4618-b68b-4d2dc2dfbfc9 · outbound

This paper cites Fourier method in the determination of rotational velocities in OB stars.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Fourier method in the determination of rotational velocities in OB stars

Reference 37

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source=arxiv_source observed=2026-08-15T14:18:44.776750Z digest=sha256:7f3a87dec9cc118d9b19650adf44a03c704cf5779acca4c24ff1b0be19fc7511

Observation 9c9ebd82-5e1c-4827-b417-c3c08554fe4a · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 38

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source=arxiv_source observed=2026-08-15T14:18:44.821582Z digest=sha256:89a0b397cfa14839d30dd8ac596bbfcae942f7b9e9c42baa2c04b315bea247ff

Observation c4ed2469-5ad9-4988-9fd5-2c8f1dffb28a · outbound

This paper cites Soviet Astronomy Letters , year = 1984, month = oct, volume =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Soviet Astronomy Letters , year = 1984, month = oct, volume =

Reference 39

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no resolver link, observed 2026-08-15T14:18:44.957960Z

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source=arxiv_source observed=2026-08-15T14:18:44.957960Z digest=sha256:462cea3b96ff6732fec43d8c45f30031bd63a81f865794dd4ea9e0bbe81ebfa3

Observation dc7ed0f8-1749-4bd8-b23c-43bb7f4b8a81 · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 40

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no resolver link, observed 2026-08-15T14:18:44.963862Z

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source=arxiv_source observed=2026-08-15T14:18:44.963862Z digest=sha256:aed25bc6d71162aba4ad7f9faa9e933a7433ff55cdee71f11803d0df6eb63018

Observation 1bd17f49-2f81-4ccc-9f12-4ac7902d4216 · outbound

This paper cites The Galactic O-Star Spectroscopic Survey. I. Classification System and Bright Northern Stars in the Blue-Violet at R~2500.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants The Galactic O-Star Spectroscopic Survey. I. Classification System and Bright Northern Stars in the Blue-Violet at R~2500

Reference 41

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no resolver link, observed 2026-08-15T14:18:45.091460Z

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source=arxiv_source observed=2026-08-15T14:18:45.091460Z digest=sha256:1331762a552d61831887ba500726c32f8e864b7b91be4ae512d48b0f10b3a90c

Observation 60b0ef15-2945-4959-8393-30e80eadfe09 · outbound

This paper cites MONOS: Multiplicity Of Northern O-type Spectroscopic systems. I. Project description and spectral classifications and visual multiplicity of previously known objects.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants MONOS: Multiplicity Of Northern O-type Spectroscopic systems. I. Project description and spectral classifications and visual multiplicity of previously known objects

Reference 42

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no resolver link, observed 2026-08-15T14:18:45.117612Z

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source=arxiv_source observed=2026-08-15T14:18:45.117612Z digest=sha256:2d8559c1e9e82704d650a775144b180e89525dce915151754e1831a13f57a26c

Observation ba75396f-71ac-4b4f-ad3a-47aafc8d8f2f · outbound

This paper cites A new calibration of stellar parameters of Galactic O stars.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants A new calibration of stellar parameters of Galactic O stars

Reference 43

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no resolver link, observed 2026-08-15T14:18:45.167877Z

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source=arxiv_source observed=2026-08-15T14:18:45.167877Z digest=sha256:42610130176cb2ee5684c2c480c473c063798581d25051f85ccfc99c15d1fe7b

Observation 92a3f511-d84a-4242-b3a1-f343d5ae9c27 · outbound

This paper cites New self-consistent wind parameters fitting optical spectra of O-type stars observed with HERMES spectrograph.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants New self-consistent wind parameters fitting optical spectra of O-type stars observed with HERMES spectrograph

Reference 44

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no resolver link, observed 2026-08-15T14:18:45.235860Z

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source=arxiv_source observed=2026-08-15T14:18:45.235860Z digest=sha256:11dab281458ff6b29883de1ac3ef537653e1295a6792b0a1a173646e140b7338

Observation fd366b30-8e98-4b1a-9522-189fdbe4f200 · outbound

This paper cites The IACOB project. VII. The rotational properties of Galactic massive O-type stars revisited.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants The IACOB project. VII. The rotational properties of Galactic massive O-type stars revisited

Reference 45

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no resolver link, observed 2026-08-15T14:18:45.342744Z

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source=arxiv_source observed=2026-08-15T14:18:45.342744Z digest=sha256:3996844fa1533bb20294c507e3395d0a7af80e5cd483d051cedba591ef3d2d27

Observation 033d2024-094e-4dda-95ca-385a3fd9d492 · outbound

This paper cites The IACOB project. V. Spectroscopic parameters of the O-type stars in the modern grid of standards for spectral classification.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants The IACOB project. V. Spectroscopic parameters of the O-type stars in the modern grid of standards for spectral classification

Reference 46

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no resolver link, observed 2026-08-15T14:18:45.376516Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-15T14:18:45.376516Z digest=sha256:b44a90ba594aee5ac29bab8bbf5eb2862fc51eb8e24d4b3f03deefa7336f8d78

Observation 1ac7d98b-b4ee-40d5-9200-a55191f668a6 · outbound

This paper cites The IACOB project: I. Rotational velocities in Northern Galactic O and early B-type stars revisited. The impact of other sources of line-broadening.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants The IACOB project: I. Rotational velocities in Northern Galactic O and early B-type stars revisited. The impact of other sources of line-broadening

Reference 47

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no resolver link, observed 2026-08-15T14:18:45.384040Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-15T14:18:45.384040Z digest=sha256:4754fcdf9ba87937f7c39f15f11bbcd022c4a1e6db7852d1364f0b4221d5dca6

Observation 2d20c17e-4740-4111-88ff-1206763ec106 · outbound

This paper cites Period spacings of $\gamma$ Doradus pulsators in the \textit{Kepler} field: Rossby and gravity modes in 82 stars.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Period spacings of $\gamma$ Doradus pulsators in the \textit{Kepler} field: Rossby and gravity modes in 82 stars

Reference 48

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unresolved
no resolver link, observed 2026-08-15T14:18:45.492324Z

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source=arxiv_source observed=2026-08-15T14:18:45.492324Z digest=sha256:ea2bee2df248a552430a7329d62b58c580b8b3b1519725f2cdaf18beabc86423

Observation dcd09c6e-4b7f-48ae-83b4-1bbef6c51f5f · outbound

This paper cites KIC~8975515: a fast-rotating ($\gamma$ Dor - $\delta$ Sct) hybrid star with Rossby modes and a slower $\delta$ Sct companion in a long-period orbit.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants KIC~8975515: a fast-rotating ($\gamma$ Dor - $\delta$ Sct) hybrid star with Rossby modes and a slower $\delta$ Sct companion in a long-period orbit

Reference 49

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no resolver link, observed 2026-08-15T14:18:45.497943Z

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source=arxiv_source observed=2026-08-15T14:18:45.497943Z digest=sha256:a2e07e3d3a992620741ad46358c87dbb5741d3b4f3b25e1cc1c5127220dd7d33

Observation 5bae1aa9-570b-404f-90fa-50851723fae8 · outbound

This paper cites Progress of Seismology of the Sun and Stars , year = 1990, editor =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Progress of Seismology of the Sun and Stars , year = 1990, editor =

Reference 50

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unresolved
no resolver link, observed 2026-08-15T14:18:45.608565Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-15T14:18:45.608565Z digest=sha256:ffb9a52d2a4334d0ba5ec15a44b41fbb1c1038c05fe8d0c077f3f5b690b529bc

Observation 655e0553-3a7d-4bed-912a-93c5a92edde0 · outbound

This paper cites Extension of the - diagram.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Extension of the - diagram

Reference 51

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no resolver link, observed 2026-08-15T14:18:45.613323Z

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source=arxiv_source observed=2026-08-15T14:18:45.613323Z digest=sha256:3e9540232318a61646a163b68d050d294580b0e661391c2ccf4df3e1aa6fbeb7

Observation c9eb9397-4789-4583-9fd2-2f0680a4d681 · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 52

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no resolver link, observed 2026-08-15T14:18:45.785338Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-15T14:18:45.785338Z digest=sha256:f92d86da822fa9af43d8b2f370cf1a0186319aacab28255e66d94b838dd24a54

Observation 104f9271-92b2-4ca2-a6b6-6f7c62ef1258 · outbound

This paper cites The interior rotation of a sample of gamma Doradus stars from ensemble modelling of their gravity mode period spacings.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants The interior rotation of a sample of gamma Doradus stars from ensemble modelling of their gravity mode period spacings

Reference 53

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no resolver link, observed 2026-08-15T14:18:45.790737Z

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source=arxiv_source observed=2026-08-15T14:18:45.790737Z digest=sha256:16c242b750aaef26e3e85af67fe5e243c8127bc5d973d8b735a6bfe667ae24c0

Observation 443ed8da-065d-4179-a7eb-4884e3e458c8 · outbound

This paper cites Properties of Galactic early-type O-supergiants: A combined FUV-UV and optical analysis.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Properties of Galactic early-type O-supergiants: A combined FUV-UV and optical analysis

Reference 54

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no resolver link, observed 2026-08-15T14:18:45.951184Z

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source=arxiv_source observed=2026-08-15T14:18:45.951184Z digest=sha256:2256f168ccbeecc6209217f42d10160803cd536bf8677047cbf7007d92e45c8d

Observation b3e8189c-f6c6-4f7b-88df-dcd08f7b44e6 · outbound

This paper cites Empirical mass-loss rates and clumping properties of Galactic early-type O supergiants.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Empirical mass-loss rates and clumping properties of Galactic early-type O supergiants

Reference 55

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no resolver link, observed 2026-08-15T14:18:45.957586Z

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source=arxiv_source observed=2026-08-15T14:18:45.957586Z digest=sha256:27334bdf9fb7a73b884e3f887f8e10a39caa243cd60506b698ab440508c251f9

Observation 3c598ad9-f470-47ed-b752-8d81d5366a57 · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 56

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no resolver link, observed 2026-08-15T14:18:46.059792Z

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source=arxiv_source observed=2026-08-15T14:18:46.059792Z digest=sha256:b78f848f0e641107fc1cafaa7b5f1dd74ee9d847c9d6b435c9b5e1639ed13409

Observation da2edfb8-bdfb-4310-adb9-10dca90afe72 · outbound

This paper cites Quantitative spectral classification of Galactic O stars.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Quantitative spectral classification of Galactic O stars

Reference 57

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no resolver link, observed 2026-08-15T14:18:46.065234Z

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source=arxiv_source observed=2026-08-15T14:18:46.065234Z digest=sha256:38d2ed4cd7262fbd828a00a449de9f23310a3d795a83172fef9c268f573f9282

Observation 2d5083e2-95d1-4384-8194-5fe6d84a5675 · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 58

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no resolver link, observed 2026-08-15T14:18:46.123364Z

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source=arxiv_source observed=2026-08-15T14:18:46.123364Z digest=sha256:9f92846951f92e0a581f6c2cca696d5a5b6fb3f66d4291457c9d901c54b23c5e

Observation ed8c0d8e-b1ae-4509-ab27-23c14c551b87 · outbound

This paper cites SF2A-2018: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics , year = 2018, editor =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants SF2A-2018: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics , year = 2018, editor =

Reference 59

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no resolver link, observed 2026-08-15T14:18:46.128918Z

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source=arxiv_source observed=2026-08-15T14:18:46.128918Z digest=sha256:65db210cb1e0e6dc911e8eb5ca58f8d2a05215e94d91874e258e06ca4accc889

Observation af3bba81-2d2a-4ec2-b7f7-8bb7b70a1015 · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 60

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source=arxiv_source observed=2026-08-15T14:18:46.133889Z digest=sha256:e360f95c0a24ef442a22dd73f6c2a1e583de60bbfe9ba58343a78ddd5b52e313

Observation e45e89c0-ed9a-4a02-9e10-38b3244cf19e · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 61

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no resolver link, observed 2026-08-15T14:18:46.220693Z

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source=arxiv_source observed=2026-08-15T14:18:46.220693Z digest=sha256:c7e3b31aa236f52f02d5b978d7751da5fd4ee1932b8566a49b75f45109cadfb9

Observation 1b38c379-4e96-46f9-a0e1-0f974e67fa18 · outbound

This paper cites , year = 1972, month = may, volume =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , year = 1972, month = may, volume =

Reference 62

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no resolver link, observed 2026-08-15T14:18:46.226160Z

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source=arxiv_source observed=2026-08-15T14:18:46.226160Z digest=sha256:e6c3b83dc0082cbe1fe5cb73ccec770cc44fddbe9ac1ca961a8edfa8f44ba0b1

Observation 840c4eb9-04f4-4461-b70f-018ff6ca3f34 · outbound

This paper cites Gaia Data Release 2: The astrometric solution.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Gaia Data Release 2: The astrometric solution

Reference 63

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no resolver link, observed 2026-08-15T14:18:46.276833Z

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source=arxiv_source observed=2026-08-15T14:18:46.276833Z digest=sha256:23d72f9b0cb96d7e7da2b02a402da70d40d0a53af4f87d137e091047d611e200

Observation 6ef98eac-0a46-4c03-932c-16d80fe323fc · outbound

This paper cites Communications in Asteroseismology , year = 2005, month = jun, volume =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Communications in Asteroseismology , year = 2005, month = jun, volume =

Reference 64

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no resolver link, observed 2026-08-15T14:18:46.282191Z

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source=arxiv_source observed=2026-08-15T14:18:46.282191Z digest=sha256:6677d0f642fc876093caf7cb325fc81ac7cd0e7e71c198d7d2e04fe21bc9e323

Observation b74780b0-a750-4dfe-963b-ad69e8c3148c · outbound

This paper cites 10.1051/0004-6361/201526154.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants 10.1051/0004-6361/201526154

Reference 65

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no resolver link, observed 2026-08-15T14:18:46.373653Z

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source=arxiv_source observed=2026-08-15T14:18:46.373653Z digest=sha256:7c9de84bba594e2c2f788ecc016a4baffb6d14b7f4da4eb68ff1986846355390

Observation f4d65468-3282-4dfc-b0ea-7191c5699359 · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 66

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no resolver link, observed 2026-08-15T14:18:46.379439Z

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source=arxiv_source observed=2026-08-15T14:18:46.379439Z digest=sha256:5e957e716c0bbdf3f8a2f57bda7e74cda9bf13f0182c8af1805e06f5bf6454fb

Observation 9a7e007b-d5ea-4a4f-8e89-41fcfed6dcb0 · outbound

This paper cites Spectroscopic study of the O-type runaway supergiant HD 195592.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Spectroscopic study of the O-type runaway supergiant HD 195592

Reference 67

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no resolver link, observed 2026-08-15T14:18:46.463003Z

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source=arxiv_source observed=2026-08-15T14:18:46.463003Z digest=sha256:440746448e8afc13f8842b5ab99add86bb7ff981db1ecc71ac386f3fcfa8cf9f

Observation cb22d3c1-27ec-413b-864f-0d4f44f34f0b · outbound

This paper cites A Spectroscopic Study of Field and Runaway OB Stars.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants A Spectroscopic Study of Field and Runaway OB Stars

Reference 68

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no resolver link, observed 2026-08-15T14:18:46.566790Z

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source=arxiv_source observed=2026-08-15T14:18:46.566790Z digest=sha256:4a0dcef850e4560809024735b2636be271aea9e83bb5055dd3f91125ba1442f1

Observation aafead1b-59e6-44c4-97f6-ee77fa856166 · outbound

This paper cites Is the bowshock of the runaway massive star HD 195592 a Fermi source?.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Is the bowshock of the runaway massive star HD 195592 a Fermi source?

Reference 69

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no resolver link, observed 2026-08-15T14:18:46.572227Z

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source=arxiv_source observed=2026-08-15T14:18:46.572227Z digest=sha256:f77a5740020a113820dcf646290b99078312e97d6209828530bcb43fbeecb86e

Observation f1709931-6681-43b2-8adf-054f77791d60 · outbound

This paper cites Variability of Blue Supergiants in the LMC with TESS.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Variability of Blue Supergiants in the LMC with TESS

Reference 70

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no resolver link, observed 2026-08-15T14:18:46.719582Z

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source=arxiv_source observed=2026-08-15T14:18:46.719582Z digest=sha256:50f02671e3bb11bf4a965fc6aec5487f65fdcb6a7ab2f2005a62d48d0a40ac60

Observation 62ea026e-04cb-432e-af6f-5c596c87fca6 · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 71

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no resolver link, observed 2026-08-15T14:18:46.727579Z

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source=arxiv_source observed=2026-08-15T14:18:46.727579Z digest=sha256:aa291729911c87812db7d7f9f51cf4302803be10b007e525dfa526791af50531

Observation 2603ec94-4cbb-499a-bae0-a8f2c06cdd43 · outbound

This paper cites Stochastic Low Frequency Variability in 3-Dimensional Radiation Hydrodynamical Models of Massive Star Envelopes.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Stochastic Low Frequency Variability in 3-Dimensional Radiation Hydrodynamical Models of Massive Star Envelopes

Reference 72

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unresolved
no resolver link, observed 2026-08-15T14:18:46.838221Z

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source=arxiv_source observed=2026-08-15T14:18:46.838221Z digest=sha256:5be048863f31b9c50c557bf266db23bf96d98a584755d7de338da23d85e107cb

Observation 3292256d-1cd6-4e63-9c87-31efd7a157c1 · outbound

This paper cites 3D hydrodynamic simulations of massive main-sequence stars II. Convective excitation and spectra of internal gravity waves.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants 3D hydrodynamic simulations of massive main-sequence stars II. Convective excitation and spectra of internal gravity waves

Reference 73

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source=arxiv_source observed=2026-08-15T14:18:46.852609Z digest=sha256:0f6a4ff1e9380628442fdee50cff689d6602a96d8e440a30cdcee1e2b756f97b

Observation 2fa8d826-48af-4f9a-959c-bb6ed634bc7f · outbound

This paper cites Internal Gravity Waves in Massive Stars: Angular Momentum Transport.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Internal Gravity Waves in Massive Stars: Angular Momentum Transport

Reference 74

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no resolver link, observed 2026-08-15T14:18:46.902601Z

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source=arxiv_source observed=2026-08-15T14:18:46.902601Z digest=sha256:bee0c53043d74f4271970aa3d162a8fdbe4f029e1d149291828645bed8f64980

Observation 49656e73-65ca-456c-8369-d25059d5b7a8 · outbound

This paper cites On the Origin of Stochastic, Low-Frequency Photometric Variability in Massive Stars.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants On the Origin of Stochastic, Low-Frequency Photometric Variability in Massive Stars

Reference 75

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source=arxiv_source observed=2026-08-15T14:18:46.919595Z digest=sha256:fa6e699721c6d3412f14ecc7c51e7a233af8c283492a764b0eac016eb626b15f

Observation b483b98b-9d46-4fc8-b8a9-32b692c9e6f3 · outbound

This paper cites The Transiting Exoplanet Survey Satellite.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants The Transiting Exoplanet Survey Satellite

Reference 76

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no resolver link, observed 2026-08-15T14:18:46.995004Z

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source=arxiv_source observed=2026-08-15T14:18:46.995004Z digest=sha256:70e0b902a736d597c91e1c3977c348114219ffd43b1d08703402109f1d40f5a9

Observation 014dcbba-65be-474f-af9a-b1c4a3f3987b · outbound

This paper cites Stellar evolution with rotation VI: The Eddington and Omega-limits, the rotational mass loss for OB and LBV stars.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Stellar evolution with rotation VI: The Eddington and Omega-limits, the rotational mass loss for OB and LBV stars

Reference 77

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no resolver link, observed 2026-08-15T14:18:47.001006Z

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source=arxiv_source observed=2026-08-15T14:18:47.001006Z digest=sha256:077ce426ef8e1ef898288c7b225d7cc0eae6bae17af1d3cbb9e3df5d84ed54bc

Observation f8889ee3-7e86-481b-895d-4641183b7148 · outbound

This paper cites Understanding the Lomb-Scargle Periodogram.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Understanding the Lomb-Scargle Periodogram

Reference 78

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no resolver link, observed 2026-08-15T14:18:47.062691Z

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source=arxiv_source observed=2026-08-15T14:18:47.062691Z digest=sha256:44cae469a1985a28727930fa056c014c0a26ee580e0ebbcfdd51e12fc66d184a

Observation 802c9fb5-c26d-4738-af95-62f1681a65f7 · outbound

This paper cites Observational signatures of convectively driven waves in massive stars.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Observational signatures of convectively driven waves in massive stars

Reference 79

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no resolver link, observed 2026-08-15T14:18:47.069166Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-15T14:18:47.069166Z digest=sha256:05db717fe3e9082ed3f0501566ccc2e0b5324f6dc882fe971c67c579d92cfcd3

Observation f51f8175-265f-4d8a-a04e-3bf1e5115566 · outbound

This paper cites On the Differential Rotation of Massive Main Sequence Stars.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants On the Differential Rotation of Massive Main Sequence Stars

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-15T14:18:47.098153Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-15T14:18:47.098153Z digest=sha256:f5059756c28e58d28e7febca25ec8b5ac7e9b24209a63801c765fe0f5e7d8791

Observation 196a5c36-bf6d-4e39-8643-572909b12f33 · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 81

Resolution
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no resolver link, observed 2026-08-15T14:18:47.103865Z

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source=arxiv_source observed=2026-08-15T14:18:47.103865Z digest=sha256:8caa74ae3edbbdadc2e3e491cd4578efd5d66462acdbdd4256d7fd8d4ae18c67

Observation 07463bff-bf48-43db-accf-58964503a15b · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 82

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no resolver link, observed 2026-08-15T14:18:47.229133Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-15T14:18:47.229133Z digest=sha256:3f0a28c4f558b3b605f5fb7e17f1a60aabde4dc90845b977f11b214a1ec91a05

Observation 2f7ba461-6101-4a55-a6b2-ed8952554cc4 · outbound

This paper cites Variability of OB stars from TESS southern Sectors 1-13 and high-resolution IACOB and OWN spectroscopy.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Variability of OB stars from TESS southern Sectors 1-13 and high-resolution IACOB and OWN spectroscopy

Reference 83

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no resolver link, observed 2026-08-15T14:18:47.234084Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-15T14:18:47.234084Z digest=sha256:fc9d0ba17493fa4175fe7041d1f9c9d21d00cd997c8f78eb8dc84c7fda61edfd

Observation cd42e237-dc1f-4b8e-b3de-49a95963a7a1 · outbound

This paper cites The -slow hydrodynamic regime.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants The -slow hydrodynamic regime

Reference 84

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no resolver link, observed 2026-08-15T14:18:47.245872Z

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source=arxiv_source observed=2026-08-15T14:18:47.245872Z digest=sha256:0691177078c16a1ddbafccc85f2663a01959faa2e7e225554f223b4141956e6f

Observation 048c7239-3481-4e04-8578-50b6e0ac460a · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 85

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no resolver link, observed 2026-08-15T14:18:47.302440Z

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source=arxiv_source observed=2026-08-15T14:18:47.302440Z digest=sha256:4d68c298ef591b4a48bddd0d60550ba4a1e583a3f41e2d062c6c78ba1af1d4fe

Observation 30c95cac-c61a-4d46-bb2d-d5a715f2ff97 · outbound

This paper cites A Detection Threshold in the Amplitude Spectra Calculated from TESS Time-Series Data.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants A Detection Threshold in the Amplitude Spectra Calculated from TESS Time-Series Data

Reference 86

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no resolver link, observed 2026-08-15T14:18:47.324756Z

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source=arxiv_source observed=2026-08-15T14:18:47.324756Z digest=sha256:c9708dd92d35ec89a5aa69caf3f5f2b5443519be6bc69793586ec1cfb1a773fe

Observation d2cd4a65-cc9e-4a9a-be16-721dfd48977b · outbound

This paper cites Photometric detection of internal gravity waves in upper main-sequence stars. II. Combined TESS photometry and high-resolution spectroscopy.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Photometric detection of internal gravity waves in upper main-sequence stars. II. Combined TESS photometry and high-resolution spectroscopy

Reference 87

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no resolver link, observed 2026-08-15T14:18:47.371117Z

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source=arxiv_source observed=2026-08-15T14:18:47.371117Z digest=sha256:1d83acc019a6125453aaccc53bf71fba6d2e6fc3307f6e15cdeada90b42c15ad

Observation 36e012d6-769c-4511-842b-0f14c8a19f10 · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 88

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no resolver link, observed 2026-08-15T14:18:47.375991Z

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source=arxiv_source observed=2026-08-15T14:18:47.375991Z digest=sha256:5d918d307d53f0b9939ad62615900cf4613062225b8d13a7830240145c45da55

Observation 6c709fc9-fd0d-4d3c-bfec-27c2ddb3557c · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 89

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no resolver link, observed 2026-08-15T14:18:47.456281Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-15T14:18:47.456281Z digest=sha256:799f787ebcd6e8b22ba5310a592bedef688fc2ab886184824bf494e5889ff72a

Observation 1ea54065-9c1d-4666-a9b3-4ca901c4a4af · outbound

This paper cites The Rayleigh Criterion: Resolution Limits of Astronomical Periodograms.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants The Rayleigh Criterion: Resolution Limits of Astronomical Periodograms

Reference 90

Resolution
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no resolver link, observed 2026-08-15T14:18:47.461572Z

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source=arxiv_source observed=2026-08-15T14:18:47.461572Z digest=sha256:c242a1feda1dee078c13ad40b650a8050354257dcd215c4c1676e38f7972da1a

Observation 8917cd37-aa60-4c82-bd0f-61068a171f94 · outbound

This paper cites Grids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014).

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Grids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014)

Reference 91

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source=arxiv_source observed=2026-08-15T14:18:47.551105Z digest=sha256:0983431b5574e385b4424a0b18e1e77c477bd6e4eac82d9fa50c36717eda0ebe

Observation 91e398f1-f68f-437e-b87f-1db66aacefab · outbound

This paper cites The generalised Lomb-Scargle periodogram. A new formalism for the floating-mean and Keplerian periodograms.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants The generalised Lomb-Scargle periodogram. A new formalism for the floating-mean and Keplerian periodograms

Reference 92

Resolution
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no resolver link, observed 2026-08-15T14:18:47.556621Z

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source=arxiv_source observed=2026-08-15T14:18:47.556621Z digest=sha256:9589c073750f0690f038ff0f9dc63141b0c2d8a68bb1a6e8b15fefe737db5e85

Observation 44db6384-94c1-4bad-aaf0-47793a09f038 · outbound

This paper cites , keywords =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , keywords =

Reference 93

Resolution
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no resolver link, observed 2026-08-15T14:18:47.599525Z

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source=arxiv_source observed=2026-08-15T14:18:47.599525Z digest=sha256:fd3db6ece95ca9b669ab09b67ea78c35a1299b364ce77d9c5de4c93b2bfd35b0

Observation 739f0575-c247-4e0c-9d6d-f8c2ee9af888 · outbound

This paper cites A new asteroseismic diagnostic for internal rotation in $\gamma$ Doradus stars.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants A new asteroseismic diagnostic for internal rotation in $\gamma$ Doradus stars

Reference 94

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no resolver link, observed 2026-08-15T14:18:47.627005Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T14:18:47.627005Z digest=sha256:743c238a376a76b88234b29e66b110ddc9ee36663c05ea2734dda4796badf6e5

Observation 76ce935b-eace-4d2c-9c58-20ececbd17b1 · outbound

This paper cites , year = 1981, month = jan, volume =.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants , year = 1981, month = jan, volume =

Reference 95

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no resolver link, observed 2026-08-15T14:18:47.677538Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T14:18:47.677538Z digest=sha256:32be0cc7af4e5a4db8eeb3b47d52e0320a6681af355c3817fb066bfb54235259

Observation 6063f728-713f-44d3-babe-b99eba08cc05 · outbound

This paper cites Spectroscopic evolution of massive stars on the main sequence.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Spectroscopic evolution of massive stars on the main sequence

Reference 96

Resolution
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no resolver link, observed 2026-08-15T14:18:47.711564Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T14:18:47.711564Z digest=sha256:5abcffe3d2c32fe901b31d1bf46a67bf1c33b26e42264966f8eb68adc9d3b094

Observation 1dcdf299-f8a0-45fe-8594-a97b314d5885 · outbound

This paper cites The Potential of Asteroseismology to Resolve the Blue Supergiant Problem.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants The Potential of Asteroseismology to Resolve the Blue Supergiant Problem

Reference 97

Resolution
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no resolver link, observed 2026-08-15T14:18:47.716425Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T14:18:47.716425Z digest=sha256:7b68c55cb897c389b981b32e62b2afbae6c499c9bdbc314da04b26285b59f17c

Observation f0368378-4003-440f-bca0-3272553da90b · outbound

This paper cites Asteroseismic measurement of surface-to-core rotation in a main sequence A star, KIC 11145123.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Asteroseismic measurement of surface-to-core rotation in a main sequence A star, KIC 11145123

Reference 98

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no resolver link, observed 2026-08-15T14:18:47.809382Z

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source=arxiv_source observed=2026-08-15T14:18:47.809382Z digest=sha256:bab2ed092bf3f373d9d8dd05ba47d3ab92d15eb3a80511cc770722f0ede1ff65

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