Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Growth of Massive Molecular Cloud Filament by Accretion Flows I: Slow Shock Instability v.s. Ambipolar Diffusion
As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2310.16448.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T14:01:11.233175Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, 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
1
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 605dd15f-6855-4f50-b1ef-073189df0e02 · inbound
Ambipolar diffusion and the mass-to-flux ratio in a turbulent collapsing cloud cites this paper.
Ambipolar diffusion and the mass-to-flux ratio in a turbulent collapsing cloud Growth of Massive Molecular Cloud Filament by Accretion Flows I: Slow Shock Instability v.s. Ambipolar Diffusion
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T14:01:11.233175Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4f8bf610-2fa3-417f-a0a4-1779b6a034ab · inbound
The slope of the power spectrum of the density field in isothermal supersonic compressible turbulence cites this paper.
The slope of the power spectrum of the density field in isothermal supersonic compressible turbulence Growth of Massive Molecular Cloud Filament by Accretion Flows I: Slow Shock Instability v.s. Ambipolar Diffusion
Reference 1
- Resolution
- verified exact
- arxiv_id, observed 2026-05-09T02:39:43.023607Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.
Observation b2793f64-c449-44df-a777-85277bae5445 · inbound
The slope of the power spectrum of the density field in isothermal supersonic compressible turbulence cites this paper.
The slope of the power spectrum of the density field in isothermal supersonic compressible turbulence Growth of Massive Molecular Cloud Filament by Accretion Flows I: Slow Shock Instability v.s. Ambipolar Diffusion
Reference 1
- Resolution
- verified exact
- arxiv_id, observed 2026-05-08T18:28:58.046888Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.