Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1609.02204.
A citation records a reference. It does not transfer a finding from one paper to another.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
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 2026-08-15T14:41:13.925580Z
A source-named dated measurement, never combined with another source.
Source: cited_works
0 of 0 outbound references displayed
External citation measurements
No source-named external measurement is stored.
No outbound reference observations are available for this paper version.
Observation 3a1202d8-870e-4b3f-b3d4-1093d2c4f061 · inbound
Runaway OB stars within 1 kpc of the Sun A comprehensive search for stellar bowshock nebulae in the Milky Way: a catalog of 709 mid-infrared selected candidates
Reference 3
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 202180dd-4281-47a4-99a4-04134fe28d69 · inbound
An Halpha survey of infrared bow-shocks around OB-type stars A comprehensive search for stellar bowshock nebulae in the Milky Way: a catalog of 709 mid-infrared selected candidates
Reference 8
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 28a5524e-ef72-4ea6-a894-2d3d8268af1c · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry A comprehensive search for stellar bowshock nebulae in the Milky Way: a catalog of 709 mid-infrared selected candidates
Reference 194
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 553b28e1-519a-4275-bc12-580dbf240753 · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry A comprehensive search for stellar bowshock nebulae in the Milky Way: a catalog of 709 mid-infrared selected candidates
Reference 194
Source-reported events for the cited work
Unavailable: canonical work link unavailable.