Paper Citation Record · LEDGER

Simulating star formation in molecular cloud cores I. The influence of low levels of turbulence on fragmentation and multiplicity

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0309829.

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

pith.paper-citation-record.v1
astro-ph/0309829 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 2026-08-15T06:32:42.880941+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:44:36.761171Z

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

214
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 8a09027a-1795-4b28-a192-143d3b7bde86 · inbound

Formation of a Protostellar Multiple System via Rotational Fragmentation cites this paper.

Formation of a Protostellar Multiple System via Rotational Fragmentation Simulating star formation in molecular cloud cores I. The influence of low levels of turbulence on fragmentation and multiplicity

Reference 29

Resolution: verified exact; local_arxiv, observed 2026-06-25T20:58:21.383803Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 20896d20-409a-4b9b-9a36-4b497791da20 · inbound

Southern Massive Stars at High Angular Resolution (SMaSH+): Properties of hierarchical massive triples cites this paper.

Southern Massive Stars at High Angular Resolution (SMaSH+): Properties of hierarchical massive triples Simulating star formation in molecular cloud cores I. The influence of low levels of turbulence on fragmentation and multiplicity

Reference 93

Resolution: verified exact; local_arxiv, observed 2026-06-29T04:23:05.969023Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation cff1bcb7-24f6-4554-a47d-b2a9f0b161e4 · inbound

The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae cites this paper.

The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae Simulating star formation in molecular cloud cores I. The influence of low levels of turbulence on fragmentation and multiplicity

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-14T04:44:36.761171Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.