Paper Citation Record · LEDGER

On the nature of the bi-stability jump in the winds of early-type supergiants

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 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.

pith.paper-citation-record.v1
astro-ph/9908196 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T20:26:22.054555Z

measured 1 of 1 external citation measurements

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
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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 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 2026-08-12T06:34:41.77262+00:00.