Paper Citation Record · LEDGER

A Super-Alfvenic Model of Dark Clouds

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/9901288.

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

pith.paper-citation-record.v1
astro-ph/9901288 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-12T05:06:34.225475Z

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
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External citation measurements

380
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 3a123824-b9af-4a1a-be64-ad456bd71d7f · 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 A Super-Alfvenic Model of Dark Clouds

Reference 130

Resolution: verified exact; local_arxiv, observed 2026-05-21T03:59:31.958151Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 04922710-9de6-4819-9431-887bd463cf3e · inbound

Jet--ISM Interactions in Gaseous Disks: Simulating Kinetic Feedback in the Radio Galaxy 3C 326 N cites this paper.

Jet--ISM Interactions in Gaseous Disks: Simulating Kinetic Feedback in the Radio Galaxy 3C 326 N A Super-Alfvenic Model of Dark Clouds

Reference 53

Resolution: unresolved; no resolver link, observed 2026-07-12T05:06:34.225475Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f9a8ec19-2d98-4c2b-b9b9-3cab8595f391 · 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 A Super-Alfvenic Model of Dark Clouds

Reference 12

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 42e1dd02-0d6a-4987-abf0-094340a0672c · 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 A Super-Alfvenic Model of Dark Clouds

Reference 122

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.