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Paper Citation Record · LEDGER

Observational Constraints on the Ages of Molecular Clouds and the Star-Formation Timescale: Ambipolar-Diffusion--Controlled or Turbulence-Induced Star Formation?

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0512043.

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

pith.paper-citation-record.v1
astro-ph/0512043 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 2026-08-20T06:33:59.587034+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T12:59:58.251850Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-30T05:14:18.439599Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • malformed identifier0
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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 01d2d87a-83b0-4bae-bbb8-b0a1691acec4 · inbound

Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas cites this paper.

Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas Observational Constraints on the Ages of Molecular Clouds and the Star-Formation Timescale: Ambipolar-Diffusion--Controlled or Turbulence-Induced Star Formation?

Reference 274

Resolution
metadata mismatch
local_arxiv, observed 2026-05-22T08:11:16.124332Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d4745ade9114bde17ae023f7814cf52e53aa7268df28d6427747c381ccb93bac

Observation d06048cf-eca9-4cf1-a3b7-acc3787c0dfd · inbound

Projection Is All You Need: Interpreting Polarization Measurements in the Orion Clouds with Sub-Alfv\'enic MHD Simulations cites this paper.

Projection Is All You Need: Interpreting Polarization Measurements in the Orion Clouds with Sub-Alfv\'enic MHD Simulations Observational Constraints on the Ages of Molecular Clouds and the Star-Formation Timescale: Ambipolar-Diffusion--Controlled or Turbulence-Induced Star Formation?

Reference 7

Resolution
verified exact
local_arxiv, observed 2026-06-30T05:14:18.442212Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d897afba98ea21c6b31420dfd42f9ed75ca3a2727533678ced14cd5697cb15e5

Observation f1b0d83a-9493-4e32-b733-3e05a0981bf2 · 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 Observational Constraints on the Ages of Molecular Clouds and the Star-Formation Timescale: Ambipolar-Diffusion--Controlled or Turbulence-Induced Star Formation?

Reference 16

Resolution
unresolved
no resolver link, observed 2026-07-11T12:59:58.251850Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T12:59:58.251850Z digest=sha256:bd330b31bf55770afc45dcda73a88b4dbcf7ceaa3232ade95db1e33ce03f6db3