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Paper Citation Record · LEDGER

Bow shocks, bow waves, and dust waves. III. Diagnostics

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1904.00343.

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

pith.paper-citation-record.v1
1904.00343 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 2026-08-08T06:32:00.761636+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:57.055862Z

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 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.

source=arxiv_source observed=2026-07-31T12:04:43.200709Z digest=sha256:e2a62bd2daf6c0cba329e447fc7ffecdf7c0d16c0d28b443af62171f53bf31be

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.

source=arxiv_source observed=2026-08-07T20:40:57.055862Z digest=sha256:581f7d51388f57951f5ec7a6ebdbf73bd48efa78e4958fb19e1e76a475fb755a