Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A very massive runaway star from Cygnus OB2
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0704.0676.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:57.084545Z
A source-named dated measurement, never combined with another source.
Source: cited_works
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 ab1c959d-9c38-41d5-8380-1b016a6459c6 · inbound
Runaway OB stars within 1 kpc of the Sun cites this paper.
Runaway OB stars within 1 kpc of the Sun A very massive runaway star from Cygnus OB2
Reference 89
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T01:38:03.731698Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3ce8b89a-a53b-4c8e-9542-c1844c4436d5 · inbound
Large-scale emission from gamma-ray binaries: the case of LS 5039 cites this paper.
Large-scale emission from gamma-ray binaries: the case of LS 5039 A very massive runaway star from Cygnus OB2
Reference 88
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T23:37:49.246294Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bc7ecc81-b187-4046-9f49-ff78789a79a2 · 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 A very massive runaway star from Cygnus OB2
Reference 71
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.084545Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.