Paper Citation Record · LEDGER

Self-gravitational Magnetohydrodynamics with Adaptive Mesh Refinement for Protostellar Collapse

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0609105.

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

pith.paper-citation-record.v1
astro-ph/0609105 v3

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 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T17:19:39.755715Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 cb6135ee-4032-457b-b391-5df01e1b0ab8 · inbound

Accretion across scales: streamers, surface-layer transport, and rapid replenishment in young protoplanetary discs cites this paper.

Accretion across scales: streamers, surface-layer transport, and rapid replenishment in young protoplanetary discs Self-gravitational Magnetohydrodynamics with Adaptive Mesh Refinement for Protostellar Collapse

Reference 193

Resolution: unresolved; no resolver link, observed 2026-08-04T11:34:15.280198Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation edddc148-2c99-4963-9a79-662e98e2b215 · inbound

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation cites this paper.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Self-gravitational Magnetohydrodynamics with Adaptive Mesh Refinement for Protostellar Collapse

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.755715Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.