Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Non-thermal high-energy emission from colliding winds of massive stars
As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/0510701.
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 2026-08-22T06:32:14.747728+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T14:41:13.967013Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
134
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 8d0217bf-bf31-43da-97d3-1ee34f4cefa6 · inbound
Gamma-rays and positrons from Colliding Wind Binaries cites this paper.
Gamma-rays and positrons from Colliding Wind Binaries Non-thermal high-energy emission from colliding winds of massive stars
Reference 28
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T05:39:26.131012Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e05e0b4e-a3c9-48e1-9fe3-eb4cf8a5a7e9 · inbound
Diffuse gamma-ray emission in the vicinity of open cluster Berkeley 87 cites this paper.
Diffuse gamma-ray emission in the vicinity of open cluster Berkeley 87 Non-thermal high-energy emission from colliding winds of massive stars
Reference 52
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T22:17:49.003686Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation cbe45db6-734c-4833-bea7-cf1d5c71f9ad · inbound
A broadband view of the thermal and non-thermal emission from the embedded massive star cluster RCW 38 cites this paper.
A broadband view of the thermal and non-thermal emission from the embedded massive star cluster RCW 38 Non-thermal high-energy emission from colliding winds of massive stars
Reference 5
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T13:49:31.057518Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation d23c7489-fb7f-4fa1-8a74-5e20d3b999fb · 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 Non-thermal high-energy emission from colliding winds of massive stars
Reference 199
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.569249Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1444c46c-5505-45e6-8e40-1ef8f125d5ab · 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 Non-thermal high-energy emission from colliding winds of massive stars
Reference 199
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T14:41:13.967013Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.