Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Inefficient star formation through turbulence, magnetic fields and feedback
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1504.03690.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T04:25:51.644415Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-28T11:22:03.012912Z
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 4198d82f-f3e6-4014-9b79-fc5806d35ac1 · inbound
The Accretion Process on Protostars cites this paper.
The Accretion Process on Protostars Inefficient star formation through turbulence, magnetic fields and feedback
Reference 176
- Resolution
- verified exact
- local_arxiv, observed 2026-05-14T18:42:35.541307Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation c6d04b24-256f-400a-b522-7db692f2412d · 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 Inefficient star formation through turbulence, magnetic fields and feedback
Reference 142
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-22T08:11:16.529441Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation ba8f290f-b11b-47b7-b441-8f3586db37e7 · inbound
Centrally concentrated star formation in young clusters II: Jet feedback cites this paper.
Centrally concentrated star formation in young clusters II: Jet feedback Inefficient star formation through turbulence, magnetic fields and feedback
Reference 128
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T11:22:03.014450Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 6c7d04f7-9a38-4f92-bb56-43868db4d12d · inbound
Small-scale Magnetic Fields in the Milky Way and Nearby Galaxies cites this paper.
Small-scale Magnetic Fields in the Milky Way and Nearby Galaxies Inefficient star formation through turbulence, magnetic fields and feedback
Reference 209
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T00:48:45.311391Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 2d3926d2-5f5a-4b79-8560-f365d4a70d57 · inbound
Exploring the Magnetic Field Structure of the Milky Way with Pulsars in the SKA Era cites this paper.
Exploring the Magnetic Field Structure of the Milky Way with Pulsars in the SKA Era Inefficient star formation through turbulence, magnetic fields and feedback
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T03:20:45.570802Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 300c0278-4f6e-40c0-8a9d-4af9d15207f0 · inbound
mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy cites this paper.
mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy Inefficient star formation through turbulence, magnetic fields and feedback
Reference 151
- Resolution
- unresolved
- no resolver link, observed 2026-07-13T06:20:04.707661Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 31d7b5f1-a6f0-4650-b894-9b65d27d30b0 · inbound
Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation cites this paper.
Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Inefficient star formation through turbulence, magnetic fields and feedback
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T17:19:39.518105Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4e0b7fb5-c4ba-4ee5-b905-0f84a496f9cb · 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 Inefficient star formation through turbulence, magnetic fields and feedback
Reference 167
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T04:25:51.644415Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.