Paper Citation Record · LEDGER

The tidally induced warping, precession and truncation of accretion discs in binary systems: three-dimensional simulations

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9604013.

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

pith.paper-citation-record.v1
astro-ph/9604013 v2

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 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T20:51:29.212019Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-12T06:01:24.667660Z

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 6531a892-da92-4de2-8964-b34c3b9a81d2 · inbound

Circumstellar and circumbinary discs in multiple stellar systems cites this paper.

Circumstellar and circumbinary discs in multiple stellar systems The tidally induced warping, precession and truncation of accretion discs in binary systems: three-dimensional simulations

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-09T20:51:29.212019Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e661159c-cae4-4a52-88d2-1cecf06c3e63 · inbound

A low viscosity relatively thick twisted disk in a supermassive binary black hole as a potential model of OJ 287 cites this paper.

A low viscosity relatively thick twisted disk in a supermassive binary black hole as a potential model of OJ 287 The tidally induced warping, precession and truncation of accretion discs in binary systems: three-dimensional simulations

Reference 43

Resolution: verified exact; arxiv_id, observed 2026-07-04T20:23:11.888642Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.