Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Radiation-pressure-driven dust waves inside bursting interstellar bubbles
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1404.2807.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:56.871993Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 a0a88274-17c8-4bae-a190-d6a08247eea1 · 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 Radiation-pressure-driven dust waves inside bursting interstellar bubbles
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T12:04:43.268198Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3b58660a-940a-4a4f-9732-34bdf80725ea · inbound
Bipolar HII regions Produced by Cloud-Cloud Collisions cites this paper.
Bipolar HII regions Produced by Cloud-Cloud Collisions Radiation-pressure-driven dust waves inside bursting interstellar bubbles
Reference 72
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T15:39:29.986160Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 24856aba-da29-4d16-8a06-1e76feca385a · 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 Radiation-pressure-driven dust waves inside bursting interstellar bubbles
Reference 15
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:56.871993Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.