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Paper Citation Record · LEDGER

MeerKAT discovery of radio emission from the Vela X-1 bow shock

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2111.10159.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2111.10159 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:57.607499Z

measured 0 of 1 external citation measurements

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.

source=arxiv_source observed=2026-07-31T12:04:43.351805Z digest=sha256:e5309a2cf18c2e60e67f78c4092834ecaa01d2b2143109a710e868796fb86f49

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.

source=arxiv_source observed=2026-08-07T20:40:57.607499Z digest=sha256:94890ff98cd5535d4e4f84ee4d6b9762bdb5a5244da7105c96ba17f94e5a2acf