Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-05-10T15:05:39.672011Z
Paper Citation Record · LEDGER
OB runaway stars originating in the Vel OB1 association
As of 11 August 2026, this Paper Citation Record lists 2 of 2 outbound references and 1 inbound Pith citation observation for arXiv:2604.11988.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:56.923212Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
2 of 2 outbound references displayed
- verified exact0
- verified fuzzy1
- unresolved0
- parse uncertain0
- malformed identifier1
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 21adfa97-4b17-4aca-b47f-b5539726f94d · outbound
This paper cites (2023); 25.
OB runaway stars originating in the Vel OB1 association (2023); 25
Reference 1
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-18T08:32:30.426460Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 9c5e2546-76ec-4c27-9c9a-0cf1ef28c93a · outbound
This paper cites condensation.
OB runaway stars originating in the Vel OB1 association condensation
Reference 2
- Resolution
- malformed identifier
- raw_fallback, observed 2026-05-18T08:32:30.424253Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Pith citing papers
Observation 67b857b1-2879-46f0-a1f0-3537aee3ea37 · 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 OB runaway stars originating in the Vel OB1 association
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:56.923212Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.