Paper Citation Record · LEDGER

The Discordance of Mass-Loss Estimates for Galactic O-Type Stars

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/0510252.

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

pith.paper-citation-record.v1
astro-ph/0510252 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T14:56:13.186566Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-26T18:09:41.330368Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation be5c1d2a-e034-4c0e-a6ea-8b3751a332f5 · inbound

Evolution and final fates of massive stars cites this paper.

Evolution and final fates of massive stars The Discordance of Mass-Loss Estimates for Galactic O-Type Stars

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-08T14:56:13.186566Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0cccdbe7-304f-490c-acbb-c9a0e7d27e0b · 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 The Discordance of Mass-Loss Estimates for Galactic O-Type Stars

Reference 194

Resolution: verified exact; local_arxiv, observed 2026-06-26T18:09:41.332071Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation a7d10528-0cfa-4d2c-96d8-cc168bac370c · inbound

The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants cites this paper.

The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants The Discordance of Mass-Loss Estimates for Galactic O-Type Stars

Reference 108

Resolution: unresolved; no resolver link, observed 2026-08-03T02:40:45.193588Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 09aee18c-7325-428b-bd98-ba7fd5f8759c · 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 The Discordance of Mass-Loss Estimates for Galactic O-Type Stars

Reference 216

Resolution: unresolved; no resolver link, observed 2026-08-07T20:40:57.633322Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.