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Paper Citation Record · LEDGER

New stellar bow shocks and bubbles found around runaway stars

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2502.02658.

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

pith.paper-citation-record.v1
2502.02658 v1

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 2026-08-07T20:40:57.074330Z

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 1c59c528-c218-4e98-80c7-cebdfbd41e79 · 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 New stellar bow shocks and bubbles found around runaway stars

Reference 74

Resolution
unresolved
no resolver link, observed 2026-07-31T12:04:43.361757Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T12:04:43.361757Z digest=sha256:e1961599922d339ec3047755d72acaf394c4cc1f22cb7e4917adeaaeb2e7c9c2

Observation 3f006cb5-d3ef-4174-824e-04fe8f3833c6 · 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 New stellar bow shocks and bubbles found around runaway stars

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-07T20:40:57.074330Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T20:40:57.074330Z digest=sha256:2a29f0a3b64ec012cfce62fac01032c77b20d519d8e5cfb54e38c762d4415ae2