Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
AE Aurigae: first detection of non-thermal X-ray emission from a bow shock produced by a runaway star
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1208.6511.
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 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T14:41:14.018595Z
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 84aca480-d3af-4acf-af75-1b2a6e01b234 · 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 AE Aurigae: first detection of non-thermal X-ray emission from a bow shock produced by a runaway star
Reference 64
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T12:04:43.304548Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 13f7660e-f328-4133-b145-b70d62bb433e · 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 AE Aurigae: first detection of non-thermal X-ray emission from a bow shock produced by a runaway star
Reference 207
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.599699Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9756b746-16f7-4d24-83a4-c94b24c21ad1 · 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 AE Aurigae: first detection of non-thermal X-ray emission from a bow shock produced by a runaway star
Reference 207
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T14:41:14.018595Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.