Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
And then they were two: detection of non-thermal radio emission from the bow shocks of two runaway stars
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2204.11913.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T14:41:14.024492Z
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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- 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 7350234c-7934-4282-8aef-14d7315b41ae · 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 And then they were two: detection of non-thermal radio emission from the bow shocks of two runaway stars
Reference 75
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T12:04:43.368149Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 42615582-955b-4ae6-9fe8-a7e5add10cce · 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 And then they were two: detection of non-thermal radio emission from the bow shocks of two runaway stars
Reference 208
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.603602Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation aa59db47-4d31-40a6-87a5-2938b6e5aa7d · 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 And then they were two: detection of non-thermal radio emission from the bow shocks of two runaway stars
Reference 208
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T14:41:14.024492Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.