Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
On the nature of the bi-stability jump in the winds of early-type supergiants
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/9908196.
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 2026-08-15T20:20:09.758276Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
17
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 52c6af8e-83d7-4ef2-9313-05569e478345 · inbound
Early Post Asymptotic Giant Branch Instability: Does it Affect White Dwarf Hydrogen Envelope Mass? cites this paper.
Early Post Asymptotic Giant Branch Instability: Does it Affect White Dwarf Hydrogen Envelope Mass? On the nature of the bi-stability jump in the winds of early-type supergiants
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T20:20:09.758276Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7bf81242-d53a-458b-9e91-bf5c05cbe166 · inbound
Monte-Carlo radiation hydrodynamic simulations of line-driven disc winds: relaxing the isothermal approximation cites this paper.
Monte-Carlo radiation hydrodynamic simulations of line-driven disc winds: relaxing the isothermal approximation On the nature of the bi-stability jump in the winds of early-type supergiants
Reference 73
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T20:26:22.054555Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d5e78e25-c37a-4db7-81a3-04a8574c42cd · inbound
Implications of modern mass-loss rates for massive stars cites this paper.
Implications of modern mass-loss rates for massive stars On the nature of the bi-stability jump in the winds of early-type supergiants
Reference 123
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T15:03:33.509423Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ed860e66-8a6c-4866-826e-a665964a9018 · inbound
Stable mass transfer in massive binaries leading to merging black holes cites this paper.
Stable mass transfer in massive binaries leading to merging black holes On the nature of the bi-stability jump in the winds of early-type supergiants
Reference 99
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T14:34:32.304930Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7f4176c6-e785-4070-ba72-08977911ac93 · inbound
Can current models predict the local black hole merger rate? cites this paper.
Can current models predict the local black hole merger rate? On the nature of the bi-stability jump in the winds of early-type supergiants
Reference 226
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:02:10.580228Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.