Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
X-ray Observations of Bow Shocks around Runaway O Stars. The case of $\zeta$ Oph and BD+43$^{\circ}$3654
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1602.07805.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T14:41:13.892636Z
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 eceeb64f-13a2-4b6d-b116-dfc6235748b1 · 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 X-ray Observations of Bow Shocks around Runaway O Stars. The case of $\zeta$ Oph and BD+43$^{\circ}$3654
Reference 70
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T12:04:43.341540Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 46a4a214-fd15-4da4-81f1-cbb82afce568 · 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 X-ray Observations of Bow Shocks around Runaway O Stars. The case of $\zeta$ Oph and BD+43$^{\circ}$3654
Reference 188
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.528594Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8f762f52-5bb4-49eb-81f9-7795592f6ac1 · 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 X-ray Observations of Bow Shocks around Runaway O Stars. The case of $\zeta$ Oph and BD+43$^{\circ}$3654
Reference 188
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T14:41:13.892636Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.