Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Secular evolution of MHD wind-driven discs: analytical solutions in the expanded {\alpha}-framework
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2111.10145.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T04:25:52.208484Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-11T04:25:53.781710Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 5328d22d-7ad7-44ab-ac30-03b590dd1500 · inbound
Preferential alignment of Class 0, Class I protostellar disks in multiple systems across nine nearby molecular clouds cites this paper.
Preferential alignment of Class 0, Class I protostellar disks in multiple systems across nine nearby molecular clouds Secular evolution of MHD wind-driven discs: analytical solutions in the expanded {\alpha}-framework
Reference 199
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T02:36:38.077761Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation df95ae5c-8566-4c97-bf93-65615c55f69b · inbound
Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments cites this paper.
Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments Secular evolution of MHD wind-driven discs: analytical solutions in the expanded {\alpha}-framework
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-07-30T14:23:16.678532Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 801689ef-5a07-43fc-999c-da628e950552 · inbound
Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments cites this paper.
Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments Secular evolution of MHD wind-driven discs: analytical solutions in the expanded {\alpha}-framework
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T01:36:10.685742Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9c1f91b8-d022-42f5-a97d-dbcdbd5701dd · inbound
JWST/MIRI Detection of Molecular H$_2$ Winds from an Edge-on Class II Source HV Tau C cites this paper.
JWST/MIRI Detection of Molecular H$_2$ Winds from an Edge-on Class II Source HV Tau C Secular evolution of MHD wind-driven discs: analytical solutions in the expanded {\alpha}-framework
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T01:34:00.314788Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 608eaafa-3661-4227-a18d-329333529b1b · inbound
IPA: Morphology and Kinematics of Molecular Hydrogen Winds in Five Young Protostars across the Mass Spectrum Observed with JWST cites this paper.
IPA: Morphology and Kinematics of Molecular Hydrogen Winds in Five Young Protostars across the Mass Spectrum Observed with JWST Secular evolution of MHD wind-driven discs: analytical solutions in the expanded {\alpha}-framework
Reference 274
- Resolution
- verified exact
- local_arxiv, observed 2026-08-11T04:25:53.787667Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.