Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Zero Energy Rotating Accretion Flows near a Black Hole
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9607051.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T11:45:37.807717Z
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
132
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 82db77de-87bb-4ccb-83df-80ffa3b74c79 · inbound
A general relativistic hydrodynamic simulation code for studying advective, sub-Keplerian accretion flow onto black holes cites this paper.
A general relativistic hydrodynamic simulation code for studying advective, sub-Keplerian accretion flow onto black holes Zero Energy Rotating Accretion Flows near a Black Hole
Reference 59
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T11:45:37.807717Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e824fb78-6213-446d-a48c-76e139566de0 · inbound
Simulation based parameter space for shock in transonic, sub-Keplerian accretion flow onto non-rotating black holes cites this paper.
Simulation based parameter space for shock in transonic, sub-Keplerian accretion flow onto non-rotating black holes Zero Energy Rotating Accretion Flows near a Black Hole
Reference 76
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T09:21:48.827217Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.