Paper Citation Record · LEDGER

Simulating the formation of molecular clouds. II. Rapid formation from turbulent initial conditions

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/0605121.

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

pith.paper-citation-record.v1
astro-ph/0605121 v2

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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 2026-08-19T06:32:44.657259+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T15:30:09.539367Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T22:06:35.097435Z

Reference resolution

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External citation measurements

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Outbound references

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Pith citing papers

Observation e5f4cd21-5c74-49d1-8d56-29157d4ec274 · inbound

IRIS: Deciphering Spectral-Line Imagery of the Galactic Center by Machine-Learning on Simulations cites this paper.

IRIS: Deciphering Spectral-Line Imagery of the Galactic Center by Machine-Learning on Simulations Simulating the formation of molecular clouds. II. Rapid formation from turbulent initial conditions

Reference 54

Resolution: verified exact; local_arxiv, observed 2026-07-03T19:38:51.797494Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation da08d3fc-d0a2-4a5f-a02d-86eb88a8875a · inbound

The dynamical origin of the magnetic field distributions in compressible turbulence cites this paper.

The dynamical origin of the magnetic field distributions in compressible turbulence Simulating the formation of molecular clouds. II. Rapid formation from turbulent initial conditions

Reference 21

Resolution: verified exact; local_arxiv, observed 2026-07-09T22:06:35.098830Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 86296077-09d8-4105-8ed2-e0f8e02cd85a · inbound

Vz-GAL Dusty Star-Forming Galaxies: Revisiting the CO-H2 Conversion Factor Tension cites this paper.

Vz-GAL Dusty Star-Forming Galaxies: Revisiting the CO-H2 Conversion Factor Tension Simulating the formation of molecular clouds. II. Rapid formation from turbulent initial conditions

Reference 295

Resolution: unresolved; no resolver link, observed 2026-08-01T15:30:09.539367Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.