Paper Citation Record · LEDGER

New theoretical Mass-loss rates of O and B Stars

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:astro-ph/0008183.

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

pith.paper-citation-record.v1
astro-ph/0008183 v1

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 12 of 12 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 12 of 12 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:57.752544Z

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

Reference resolution

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External citation measurements

48
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 5c0c17f2-5eff-4cb0-8973-3329f1ffc68c · inbound

Simulations of Interacting Binary Systems -- Pathways to Radio Bright GRB Progenitors cites this paper.

Simulations of Interacting Binary Systems -- Pathways to Radio Bright GRB Progenitors New theoretical Mass-loss rates of O and B Stars

Reference 100

Resolution: metadata mismatch; local_arxiv, observed 2026-05-24T01:13:42.309681Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 58321ea7-2176-4295-8b43-7239c15799e9 · inbound

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

Massive Interacting Binaries Enhance Feedback in Star-Forming Regions New theoretical Mass-loss rates of O and B Stars

Reference 110

Resolution: unresolved; no resolver link, observed 2026-08-06T20:26:51.989797Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 325a1742-95f5-47f5-950d-af2e95bcd3e7 · inbound

Rotational Dynamics in Pulsational Pair-Instability Supernovae: Implications for Mass-Loss and Transient Events cites this paper.

Rotational Dynamics in Pulsational Pair-Instability Supernovae: Implications for Mass-Loss and Transient Events New theoretical Mass-loss rates of O and B Stars

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-06T13:02:27.837331Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3f684780-7963-47ff-82db-41882197d0f0 · inbound

The power of binaries on stripped-envelope supernovae across metallicity: uniform progenitor parameter space and persistently low ejecta masses, but subtype diversity cites this paper.

The power of binaries on stripped-envelope supernovae across metallicity: uniform progenitor parameter space and persistently low ejecta masses, but subtype diversity New theoretical Mass-loss rates of O and B Stars

Reference 195

Resolution: unresolved; no resolver link, observed 2026-08-05T14:41:22.974914Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 13b27bf4-e957-487c-b803-de4d5fde24b3 · inbound

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

Stable mass transfer in massive binaries leading to merging black holes New theoretical Mass-loss rates of O and B Stars

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-03T14:34:32.097539Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 25718844-2e88-48e9-a348-de314d6ef8b2 · inbound

Jets from Scratch: A 3D Dynamo Origin of Long Gamma-Ray Burst Jets cites this paper.

Jets from Scratch: A 3D Dynamo Origin of Long Gamma-Ray Burst Jets New theoretical Mass-loss rates of O and B Stars

Reference 101

Resolution: metadata mismatch; local_arxiv, observed 2026-06-30T22:05:05.348510Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 67bc40cb-025d-4357-9bd6-fc4ed740d550 · inbound

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

Can current models predict the local black hole merger rate? New theoretical Mass-loss rates of O and B Stars

Reference 102

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.928354Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 919267c1-5695-42f7-864a-b11d0f39372a · inbound

The effect of near-core mixing on rejuvenation and the asteroseismic properties of massive accretors cites this paper.

The effect of near-core mixing on rejuvenation and the asteroseismic properties of massive accretors New theoretical Mass-loss rates of O and B Stars

Reference 263

Resolution: verified exact; local_arxiv, observed 2026-06-27T05:40:36.383731Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation dbd4aa6e-b509-4afe-a2df-e8f17777494e · inbound

Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation cites this paper.

Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation New theoretical Mass-loss rates of O and B Stars

Reference 116

Resolution: verified exact; local_arxiv, observed 2026-06-26T09:59:18.142840Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation d44a9606-6b09-45f4-8c31-84cec4c035a3 · inbound

The location of the upper edge of the pair-instability supernovae black hole mass gap cites this paper.

The location of the upper edge of the pair-instability supernovae black hole mass gap New theoretical Mass-loss rates of O and B Stars

Reference 36

Resolution: metadata mismatch; local_arxiv, observed 2026-07-01T04:25:20.941353Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 78fc79de-c8bd-4e61-8cb0-66b071a0f775 · inbound

A Detailed Spectroscopic Study of the WN6ha + O5 Colliding-wind Binary WR 25 cites this paper.

A Detailed Spectroscopic Study of the WN6ha + O5 Colliding-wind Binary WR 25 New theoretical Mass-loss rates of O and B Stars

Reference 63

Resolution: unresolved; no resolver link, observed 2026-07-31T16:11:56.788930Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fbcebb45-ce7c-4aea-acbd-ea923fe4b915 · inbound

Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.

Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry New theoretical Mass-loss rates of O and B Stars

Reference 247

Resolution: unresolved; no resolver link, observed 2026-08-07T20:40:57.752544Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.