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Paper Citation Record · LEDGER

Gravitational contraction versus Supernova driving and the origin of the velocity dispersion-size relation in molecular clouds

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1511.05602.

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

pith.paper-citation-record.v1
1511.05602 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 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 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T20:11:25.299773Z

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

94
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation bb3caa16-0777-4b62-a491-22a05b8087f6 · inbound

The Importance of Tidal Forces in Molecular Cloud Dynamics cites this paper.

The Importance of Tidal Forces in Molecular Cloud Dynamics Gravitational contraction versus Supernova driving and the origin of the velocity dispersion-size relation in molecular clouds

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-06T20:11:25.299773Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T20:11:25.299773Z digest=sha256:bfc45c4c2d688bc899e719e0b8c0e2afb540946c5b5d5688cff8f95fa551445a

Observation 89553cce-e6b2-47e6-9497-3b32a62ed56e · inbound

Centrally concentrated star formation in young clusters II: Jet feedback cites this paper.

Centrally concentrated star formation in young clusters II: Jet feedback Gravitational contraction versus Supernova driving and the origin of the velocity dispersion-size relation in molecular clouds

Reference 112

Resolution
verified exact
local_arxiv, observed 2026-06-28T11:22:03.357407Z

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.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b102c41cf7835cb5dd4aa98b1d0c3d5ed88f8e6ba766afdb6185b42f2f065d23