Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Bow shocks, bow waves, and dust waves. III. Diagnostics
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1904.00343.
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 2026-08-20T06:33:59.587034+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T14:41:13.222609Z
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 06862593-846b-47ff-b9ff-57a55c8bf228 · 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 Bow shocks, bow waves, and dust waves. III. Diagnostics
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T12:04:43.200709Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 12d9b12c-9acf-4629-8e9c-3b9ed45a02c5 · 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 Bow shocks, bow waves, and dust waves. III. Diagnostics
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.055862Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b7b006f9-8d37-4262-a253-17ef0182a1ef · 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 Bow shocks, bow waves, and dust waves. III. Diagnostics
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T14:41:13.222609Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.