Paper Citation Record · LEDGER

Gravitational Binding and Star Formation in Molecular Clouds of the Milky Way

As of 13 August 2026, this Paper Citation Record lists 3 of 3 outbound references and 1 inbound Pith citation observation for arXiv:2508.05826.

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

pith.paper-citation-record.v1
2508.05826 v1

Coverage vector

measured 3 of 3 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-05T23:16:17.659625Z

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T11:14:51.924790Z

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

3 of 3 outbound references displayed

verified exact0
verified fuzzy3
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

0
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation 5ff032dc-97a9-4aec-aeb4-5d0272a477af · outbound

This paper cites rate-matching.

Gravitational Binding and Star Formation in Molecular Clouds of the Milky Way rate-matching

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T23:16:17.697534Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 915cdb38-33a6-4517-b4e0-c840adab070f · outbound

This paper cites # is often used to quantify the ability of a cloud to form stars. This section relates the observed and modeled values of 𝛼!.

Gravitational Binding and Star Formation in Molecular Clouds of the Milky Way # is often used to quantify the ability of a cloud to form stars. This section relates the observed and modeled values of 𝛼!

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T23:16:17.731873Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 97bb1c22-97e0-44bf-8814-39ec633ef1e8 · outbound

This paper cites # were analyzed in rings of width 1 kpc over 𝑅$%&=4−14 kpc. The virial parameter increases with 𝑅$%& by a factor ~2 in each survey. 2. The increasing trends of 𝛼!.

Gravitational Binding and Star Formation in Molecular Clouds of the Milky Way # were analyzed in rings of width 1 kpc over 𝑅$%&=4−14 kpc. The virial parameter increases with 𝑅$%& by a factor ~2 in each survey. 2. The increasing trends of 𝛼!

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T23:16:17.714623Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Pith citing papers

Observation 5ec22d8a-b42d-46e1-85c3-fd8679f70959 · inbound

Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback cites this paper.

Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback Gravitational Binding and Star Formation in Molecular Clouds of the Milky Way

Reference 88

Resolution: metadata mismatch; local_arxiv, observed 2026-08-04T11:18:57.361059Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.