Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Bright OB stars in the Galaxy - III. Constraints on the radial stratification of the clumping factor in hot star winds from a combined Halpha, IR and radio analysis
As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/0604372.
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 2026-08-23T06:30:58.430688+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T14:41:13.626007Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-26T18:09:41.395867Z
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 24e0fa6d-13c6-4d47-9ef6-c49589fb94a1 · inbound
Analyzing Stellar and Interstellar Contributions to Polarization: Modeling Approaches for Hot Stars cites this paper.
Analyzing Stellar and Interstellar Contributions to Polarization: Modeling Approaches for Hot Stars Bright OB stars in the Galaxy - III. Constraints on the radial stratification of the clumping factor in hot star winds from a combined Halpha, IR and radio analysis
Reference 40
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T15:30:22.348287Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation dc20ddbe-42c3-41c8-b405-9f7e54ab02d2 · inbound
Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI cites this paper.
Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI Bright OB stars in the Galaxy - III. Constraints on the radial stratification of the clumping factor in hot star winds from a combined Halpha, IR and radio analysis
Reference 145
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T18:09:41.397854Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.
Observation 65754ffd-360f-402b-b0b9-be6c0891bf08 · 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 Bright OB stars in the Galaxy - III. Constraints on the radial stratification of the clumping factor in hot star winds from a combined Halpha, IR and radio analysis
Reference 138
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.339840Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6d420d84-25b5-4ed6-bd11-a2f77238c0bc · 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 Bright OB stars in the Galaxy - III. Constraints on the radial stratification of the clumping factor in hot star winds from a combined Halpha, IR and radio analysis
Reference 138
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T14:41:13.626007Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.