Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
MeerKAT discovery of radio emission from the Vela X-1 bow shock
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2111.10159.
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 2026-08-15T14:41:14.032410Z
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 5870fb03-85a1-4e7e-a3da-98486bd3312f · 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 MeerKAT discovery of radio emission from the Vela X-1 bow shock
Reference 72
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T12:04:43.351805Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 637192ee-cb3f-40e7-b629-e98bb04cdef2 · 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 MeerKAT discovery of radio emission from the Vela X-1 bow shock
Reference 209
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.607499Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8c50e613-cd6a-455c-89d4-d006c7dcf64e · 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 MeerKAT discovery of radio emission from the Vela X-1 bow shock
Reference 209
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T14:41:14.032410Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.