Paper Citation Record · LEDGER

The Turbulent Shock Origin of Proto--Stellar Cores

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0011122.

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

pith.paper-citation-record.v1
astro-ph/0011122 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T12:59:58.251850Z

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
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

278
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 7342dc76-3aa2-4fe9-b4b9-2473bf5724cf · inbound

Evolution of compressed clouds formed by filament coalescence. I. Oblique collisions cites this paper.

Evolution of compressed clouds formed by filament coalescence. I. Oblique collisions The Turbulent Shock Origin of Proto--Stellar Cores

Reference 132

Resolution: verified exact; local_arxiv, observed 2026-05-21T03:59:31.955052Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 18e6d518-b18e-4864-b548-0a69be737113 · inbound

ALMA observations of Magnetic Fields in the Massive Star-forming Region IRAS 18360-0537 cites this paper.

ALMA observations of Magnetic Fields in the Massive Star-forming Region IRAS 18360-0537 The Turbulent Shock Origin of Proto--Stellar Cores

Reference 13

Resolution: unresolved; no resolver link, observed 2026-07-11T12:59:58.251850Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d4be9e1b-2071-47f5-9629-e2638081395d · inbound

Emergence of high-mass stars in complex fiber networks (EMERGE) VI. Turbulence dissipation and the formation of dense fibers cites this paper.

Emergence of high-mass stars in complex fiber networks (EMERGE) VI. Turbulence dissipation and the formation of dense fibers The Turbulent Shock Origin of Proto--Stellar Cores

Reference 123

Resolution: unresolved; no resolver link, observed 2026-07-11T07:55:39.166465Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.