Paper Citation Record · LEDGER

The stability of late-type stars close to the Eddington limit

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9710158.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
astro-ph/9710158 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T20:20:09.615574Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-10T05:30:23.456663Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

4
pith, observed 2026-08-10T05:30:23.456663Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 7dcab93a-b856-4f0a-9366-457a9e8775dc · inbound

The Effect of Rotation on Triggering S Doradus Instabilities in Luminous Blue Variables cites this paper.

The Effect of Rotation on Triggering S Doradus Instabilities in Luminous Blue Variables The stability of late-type stars close to the Eddington limit

Reference 4

Resolution: metadata mismatch; local_arxiv, observed 2026-08-07T21:25:51.720400Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation b975ee7b-3496-46c2-bb91-8819d68a6ab3 · 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? The stability of late-type stars close to the Eddington limit

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-15T20:20:09.615574Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.