Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
3D RMHD simulations of jet-wind interactions in High Mass X-ray Binaries
As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2202.11119.
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 2026-08-20T06:33:59.587034+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T14:41:14.444583Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-16T21:28:33.723908Z
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 bc183e05-cbc5-4e30-a477-70093fd6a8fa · inbound
Cygnus X-3: A variable petaelectronvolt gamma-ray source cites this paper.
Cygnus X-3: A variable petaelectronvolt gamma-ray source 3D RMHD simulations of jet-wind interactions in High Mass X-ray Binaries
Reference 76
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T21:28:33.725886Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation 1c6026a7-a3ee-4f8f-a681-2aecdf8ead0c · 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 3D RMHD simulations of jet-wind interactions in High Mass X-ray Binaries
Reference 283
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.889099Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 933e76e5-d989-4a72-adf4-a270223c2289 · 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 3D RMHD simulations of jet-wind interactions in High Mass X-ray Binaries
Reference 283
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T14:41:14.444583Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.