Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1903.07774.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:57.059981Z
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 8ea2f62c-7552-4a0e-89e8-52500c23b0dc · inbound
An Halpha survey of infrared bow-shocks around OB-type stars Bow shocks, bow waves, and dust waves. II. Beyond the rip point
Reference 18
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2f935896-90c2-43e7-a3b4-001486f83ebd · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry Bow shocks, bow waves, and dust waves. II. Beyond the rip point
Reference 64
Source-reported events for the cited work
Unavailable: canonical work link unavailable.