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Paper Citation Record · LEDGER

Wind modelling of very massive stars up to 300 solar masses

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1105.0556.

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

pith.paper-citation-record.v1
1105.0556 v2

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measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:26:10.059008Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T04:26:36.081650Z

Reference resolution

0 of 0 outbound references displayed

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 3279a0c7-52f3-414f-b604-f1cc8cdcfffb · inbound

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

Can current models predict the local black hole merger rate? Wind modelling of very massive stars up to 300 solar masses

Reference 98

Resolution
verified exact
local_arxiv, observed 2026-06-28T13:02:10.596292Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:7f0768c0e2df5a531bee7a38791a1c60a82ac621d4dd41f505e4aa828f067179

Observation ff6a3ba5-a849-440e-842b-5e95b4e764f8 · inbound

Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors cites this paper.

Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors Wind modelling of very massive stars up to 300 solar masses

Reference 92

Resolution
verified exact
local_arxiv, observed 2026-07-02T04:26:36.082979Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-06-28T09:07:09.699995Z digest=sha256:e9436a45c72e3aa27be98f8cfa54781db2735eed25e1f3caf4005b45aaf9101a

Observation b15158e4-5c4a-4e43-8f5b-e48be0f0838b · inbound

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI cites this paper.

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI Wind modelling of very massive stars up to 300 solar masses

Reference 180

Resolution
verified exact
local_arxiv, observed 2026-06-26T18:09:41.352457Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:145fada5ed4d892166c88dcb0f8309b1bde081997b40923a1321376214555d07

Observation 382ecbf2-cf94-4e78-84a7-919b60a37c36 · inbound

The Stellar Winds Atlas II: Black Hole Formation at Solar Metallicity cites this paper.

The Stellar Winds Atlas II: Black Hole Formation at Solar Metallicity Wind modelling of very massive stars up to 300 solar masses

Reference 278

Resolution
unresolved
no resolver link, observed 2026-08-01T00:42:46.093169Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:42:46.093169Z digest=sha256:723be2a1fb2f3c501acfae6e14120ec3b4fbd228690eafbbb4928b6181ab7c84

Observation ee270b47-368c-4328-ba32-f2aa783f7eba · inbound

SPURS: Massive Stars, Dense Gas, and Ly$\alpha$ Escape in GN-z11 at $z = 10.6$ cites this paper.

SPURS: Massive Stars, Dense Gas, and Ly$\alpha$ Escape in GN-z11 at $z = 10.6$ Wind modelling of very massive stars up to 300 solar masses

Reference 133

Resolution
unresolved
no resolver link, observed 2026-08-16T04:26:10.059008Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T04:26:10.059008Z digest=sha256:55cd5a3f8511c6a50349055dbbc5af7d45217204d47f7fff93a616f0ddd05851