Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Kinematics of the Central Stars Powering Bowshock Nebulae and the Large Multiplicity Fraction of Runaway OB Stars
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2206.09281.
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 2026-08-07T20:40:57.043382Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
0 of 0 outbound references displayed
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- 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 86848464-ba1d-4525-af30-f6973aa9ce79 · inbound
Runaway OB stars within 1 kpc of the Sun cites this paper.
Runaway OB stars within 1 kpc of the Sun Kinematics of the Central Stars Powering Bowshock Nebulae and the Large Multiplicity Fraction of Runaway OB Stars
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T01:37:59.088539Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b8430235-b149-4934-91b5-c4b79911cbcd · inbound
An Halpha survey of infrared bow-shocks around OB-type stars cites this paper.
An Halpha survey of infrared bow-shocks around OB-type stars Kinematics of the Central Stars Powering Bowshock Nebulae and the Large Multiplicity Fraction of Runaway OB Stars
Reference 106
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T12:04:43.566791Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d9eae649-b895-4d8f-a23e-d6a90b9083cd · 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 Kinematics of the Central Stars Powering Bowshock Nebulae and the Large Multiplicity Fraction of Runaway OB Stars
Reference 60
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.043382Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.