Paper Citation Record · LEDGER

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

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:astro-ph/0006405.

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

pith.paper-citation-record.v1
astro-ph/0006405 v1

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measured 0 of 0 reference resolution

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measured 11 of 11 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T10:56:57.265046Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

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External citation measurements

4
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation e00e7ec8-6e57-4e18-bb0f-06d46c30d083 · inbound

Basic stellar observables cites this paper.

Basic stellar observables Stellar evolution with rotation VI: The Eddington and Omega-limits, the rotational mass loss for OB and LBV stars

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-11T20:31:57.337036Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0ea1d683-6015-480b-8e40-418c156f5981 · inbound

Globular cluster formation from inertial inflows: accreting extremely massive stars as the origin of abundance anomalies cites this paper.

Globular cluster formation from inertial inflows: accreting extremely massive stars as the origin of abundance anomalies Stellar evolution with rotation VI: The Eddington and Omega-limits, the rotational mass loss for OB and LBV stars

Reference 159

Resolution: unresolved; no resolver link, observed 2026-08-10T17:33:44.489115Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 803c57bf-5d7c-4966-98ea-f928c46b3735 · inbound

The black hole - pair instability boundary for high stellar rotation cites this paper.

The black hole - pair instability boundary for high stellar rotation Stellar evolution with rotation VI: The Eddington and Omega-limits, the rotational mass loss for OB and LBV stars

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-16T10:56:57.265046Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c32df462-9581-4db0-946f-366063c553a6 · inbound

pySTARBURST99: The Next Generation of STARBURST99 cites this paper.

pySTARBURST99: The Next Generation of STARBURST99 Stellar evolution with rotation VI: The Eddington and Omega-limits, the rotational mass loss for OB and LBV stars

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-07T12:35:47.236804Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f2bd3b4d-fc80-4fb6-9ed5-6a6d1793d5c9 · inbound

The Gaia-ESO Survey: Projected Rotational Velocities of B stars in the Carina Nebula cites this paper.

The Gaia-ESO Survey: Projected Rotational Velocities of B stars in the Carina Nebula Stellar evolution with rotation VI: The Eddington and Omega-limits, the rotational mass loss for OB and LBV stars

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:37.690928Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8c04dcb6-cac2-4a70-9ff1-6cf1f6f6aa25 · inbound

How Dust Models Shape High-z Galaxy Morphology: Insights from the NewCluster Simulation cites this paper.

How Dust Models Shape High-z Galaxy Morphology: Insights from the NewCluster Simulation Stellar evolution with rotation VI: The Eddington and Omega-limits, the rotational mass loss for OB and LBV stars

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-05T16:33:10.113360Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation faa56bd2-73a1-43ba-a24b-7a19fc9be024 · inbound

On the Origin of Intracluster Light based on the High-resolution Simulation, NewCluster cites this paper.

On the Origin of Intracluster Light based on the High-resolution Simulation, NewCluster Stellar evolution with rotation VI: The Eddington and Omega-limits, the rotational mass loss for OB and LBV stars

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-03T18:16:57.686094Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fd87c9e3-597f-4713-9d2a-653bbf8309d4 · inbound

Can current models predict the local black hole merger rate? cites this paper.

Can current models predict the local black hole merger rate? Stellar evolution with rotation VI: The Eddington and Omega-limits, the rotational mass loss for OB and LBV stars

Reference 134

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.779726Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation e2e2d4d4-c3f9-4b71-a911-ae085fae39d0 · inbound

Accretion of Primordial Black Holes in Stellar Interiors cites this paper.

Accretion of Primordial Black Holes in Stellar Interiors Stellar evolution with rotation VI: The Eddington and Omega-limits, the rotational mass loss for OB and LBV stars

Reference 236

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:22:15.664233Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 8dcd460e-2ebf-4a65-9923-535c30fd5c94 · inbound

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants cites this paper.

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

Resolution: unresolved; no resolver link, observed 2026-08-12T12:11:54.370152Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants cites this paper.

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.