Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Galactic runaway O and Be stars found using Gaia DR3
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2311.01827.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T14:41:13.196038Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
0 of 0 outbound references displayed
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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 15f229f3-3432-4c14-9e60-18ca20c151f9 · inbound
Runaway OB stars within 1 kpc of the Sun cites this paper.
Runaway OB stars within 1 kpc of the Sun Galactic runaway O and Be stars found using Gaia DR3
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T01:37:58.787424Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b3c059b7-6465-4975-9366-e22a0f24caa3 · inbound
Large-scale emission from gamma-ray binaries: the case of LS 5039 cites this paper.
Large-scale emission from gamma-ray binaries: the case of LS 5039 Galactic runaway O and Be stars found using Gaia DR3
Reference 75
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T23:37:47.506079Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8b7b1966-10ce-43f8-98c9-bc3240291580 · 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 Galactic runaway O and Be stars found using Gaia DR3
Reference 73
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T12:04:43.356946Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c1488e50-8b8c-4ef8-a509-664d90ae62c9 · inbound
The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars cites this paper.
The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars Galactic runaway O and Be stars found using Gaia DR3
Reference 44
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T13:33:06.380063Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7318eb3e-7552-41b6-bc9a-2b63c378eb87 · 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 Galactic runaway O and Be stars found using Gaia DR3
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.035282Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cdd41b9a-75d9-455f-98b9-1f3f36f20ad7 · 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 Galactic runaway O and Be stars found using Gaia DR3
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T14:41:13.196038Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.