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Paper Citation Record · LEDGER

The Evolution of Massive Binary Stars

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2311.01865.

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

pith.paper-citation-record.v1
2311.01865 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T18:54:21.964350Z

measured 1 of 1 external citation measurements

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

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

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

3
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation eadc999d-25e1-4162-82a9-4023bafacc89 · inbound

Giants, Supergiants and Hypergiants cites this paper.

Giants, Supergiants and Hypergiants The Evolution of Massive Binary Stars

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-06T18:54:21.964350Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T18:54:21.964350Z digest=sha256:2409f26d295e1dd7f8cbf97032ecdb031b2c8443f8d06b4cb3c639653f6a737e

Observation 03add04b-4e6d-4c8d-8128-204dc89cffcd · inbound

Stellar evolution through the Red Supergiant phase cites this paper.

Stellar evolution through the Red Supergiant phase The Evolution of Massive Binary Stars

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-06T15:25:31.761763Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T15:25:31.761763Z digest=sha256:6ad3da4acfc6fbecfd1fc51cc7e627007c1fb6311004dda188dc268147513d29

Observation b8efcb53-62ee-406c-83f9-0175a37d37fb · inbound

Exploring the astrophysical origins of binary black holes using normalising flows cites this paper.

Exploring the astrophysical origins of binary black holes using normalising flows The Evolution of Massive Binary Stars

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-05T15:53:31.653191Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T15:53:31.653191Z digest=sha256:ae41746293841a67740c540c0c82b8bf8dafabac241233c62656cee9fc222d22

Observation abb1d418-a8bd-4307-8b9c-87c414470260 · 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 The Evolution of Massive Binary Stars

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-03T14:34:23.902856Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T14:34:23.902856Z digest=sha256:98246859e4d7afbea82ac76338bb7e538385cb9be4b19d2410ffdbbc142dc6d0

Observation 6821f459-24eb-4440-9bc5-638ab3505ebc · inbound

Mergers via failed common envelope as a route towards intermediate-mass stripped stars cites this paper.

Mergers via failed common envelope as a route towards intermediate-mass stripped stars The Evolution of Massive Binary Stars

Reference 60

Resolution
verified exact
arxiv_id, observed 2026-05-25T02:20:13.875922Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-05-25T02:17:35.155773Z digest=sha256:495d4f2c347837c3484523b074ab24ed1c35451c04566b88fd007dd72dd107d8

Observation 19f9de98-e93a-49f9-9195-276a86f5e7c8 · inbound

Collective Winds of Massive Star Clusters as the Dominant PeVatrons for Galactic Cosmic Rays cites this paper.

Collective Winds of Massive Star Clusters as the Dominant PeVatrons for Galactic Cosmic Rays The Evolution of Massive Binary Stars

Reference 52

Resolution
verified exact
arxiv_id, observed 2026-07-01T20:06:11.971973Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-28T21:39:08.628584Z digest=sha256:475b003c8d8d47053354792f6c3b03157ac383f9bbe524fc29348de64543ac05

Observation 08b4b6db-b39b-41e9-9aad-bb65cf6b199e · inbound

The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry cites this paper.

The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry The Evolution of Massive Binary Stars

Reference 117

Resolution
unresolved
no resolver link, observed 2026-08-05T20:04:25.543118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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