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Paper Citation Record · LEDGER

Blowing in the wind: The dust wave surrounding $\sigma$ Ori AB

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1401.7185.

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

pith.paper-citation-record.v1
1401.7185 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 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:56.848657Z

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 e05a9614-6a97-4d74-ad9a-ffcc2bd29eb7 · 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 Blowing in the wind: The dust wave surrounding $\sigma$ Ori AB

Reference 57

Resolution
unresolved
no resolver link, observed 2026-07-31T12:04:43.262540Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T12:04:43.262540Z digest=sha256:c76c2d460ebb3c07e1688def050e86952ab46e3f75bec7fc9af4d659c1d2a269

Observation c343bbd1-4545-4369-a239-cec400c08f12 · 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 Blowing in the wind: The dust wave surrounding $\sigma$ Ori AB

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-07T20:40:56.848657Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T20:40:56.848657Z digest=sha256:54599427df299f7c3f762535b5ea81dd0485a351fc91a8784e2d1b02ecdc940c