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Paper Citation Record · LEDGER

Control of star formation by supersonic turbulence

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:astro-ph/0301093.

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

pith.paper-citation-record.v1
astro-ph/0301093 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 11 of 11 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T11:34:03.303305Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T22:06:35.118867Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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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 1a064f56-ec00-45bc-92c9-438d03adfaa4 · inbound

The magnetic field of the Milky Way: an observational perspective cites this paper.

The magnetic field of the Milky Way: an observational perspective Control of star formation by supersonic turbulence

Reference 226

Resolution
metadata mismatch
local_arxiv, observed 2026-06-28T14:02:16.886104Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:31a8b14f82503d7c168825c461fa088166eec8fa54caf57873e46adcc68f9880

Observation ad6d7f51-b896-442d-b9a5-9a9dcf4a43ad · inbound

The efficiency per free-fall time as a ratio of the Star Formation Rate to the gas-infall rate in collapsing cores: dependence on the core definition, accretion, and radial structure cites this paper.

The efficiency per free-fall time as a ratio of the Star Formation Rate to the gas-infall rate in collapsing cores: dependence on the core definition, accretion, and radial structure Control of star formation by supersonic turbulence

Reference 30

Resolution
metadata mismatch
local_arxiv, observed 2026-06-26T11:59:27.224607Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b78b5db4b1dc8d12c4784ceebf2a91b80c025edb66d2660ee0170f4931ea47ce

Observation f927d22c-e35c-4aca-913e-456f23991814 · inbound

Substructures in Planet-Forming Disks with the SKAO cites this paper.

Substructures in Planet-Forming Disks with the SKAO Control of star formation by supersonic turbulence

Reference 19

Resolution
metadata mismatch
local_arxiv, observed 2026-06-25T19:38:18.225257Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:3f6349ee481b9e39063e9575ff91bd2ca77a0cfc046b9735e3152b59be15a2ec

Observation c2a98dd0-2b27-4622-8f5b-f3ce2a0cd55c · inbound

Substructures in Planet-Forming Disks with the SKAO cites this paper.

Substructures in Planet-Forming Disks with the SKAO Control of star formation by supersonic turbulence

Reference 19

Resolution
metadata mismatch
local_arxiv, observed 2026-06-29T05:03:09.339300Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:430164c42ddb82748513460a5a77eccb04a17661b162cb72e039cf946b77710f

Observation 81d0aa19-8a0c-4c38-ac9a-562869224f09 · 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 Control of star formation by supersonic turbulence

Reference 8

Resolution
metadata mismatch
local_arxiv, observed 2026-06-30T05:14:18.715803Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:714adacfafabd6a98c7b31a177e5d1627b8c603f30140b679721056219cf5a04

Observation 988a992d-d9c2-4ae6-a436-9af5c6f20ca5 · inbound

On the Eccentricity Distribution and Tidal Evolution of Transiting Brown Dwarfs cites this paper.

On the Eccentricity Distribution and Tidal Evolution of Transiting Brown Dwarfs Control of star formation by supersonic turbulence

Reference 215

Resolution
unresolved
no resolver link, observed 2026-07-12T07:45:39.933353Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T07:45:39.933353Z digest=sha256:3a76a3c68c782ea9f9bbaf230dfb0b6e42adb4332c8b9a19b5a789e10f7110ee

Observation 7931cb21-f82f-4335-9315-948df4be99ce · 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 Control of star formation by supersonic turbulence

Reference 101

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=sha256:12eb1f60aa8071d4d865675dc803c3cfb3b71590625a5421acfb1b68a4e7b05e

Observation d3a2863d-2a9b-4f8a-a185-8ca780d49885 · inbound

The dynamical origin of the magnetic field distributions in compressible turbulence cites this paper.

The dynamical origin of the magnetic field distributions in compressible turbulence Control of star formation by supersonic turbulence

Reference 30

Resolution
metadata mismatch
local_arxiv, observed 2026-07-09T22:06:35.120520Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:f4d92605c53a13695a617e9bf6d783c181864d896411dabdf206f0f6d6eb2b88

Observation b81992d6-7330-4cf8-8d06-c687d5b7f06f · 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 Control of star formation by supersonic turbulence

Reference 109

Resolution
unresolved
no resolver link, observed 2026-07-13T06:20:04.707661Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-13T06:20:04.707661Z digest=sha256:87d365155e9eb81e6d747d20dc8bae50abfc026bf456d5a36afee66d2dc81a34

Observation b141a27e-4241-484c-b3be-913dc7d08b4e · inbound

Characterising the Kinematics and Evolution of Young Stellar Groups within 1 kpc of the Sun Using Gaia DR3 cites this paper.

Characterising the Kinematics and Evolution of Young Stellar Groups within 1 kpc of the Sun Using Gaia DR3 Control of star formation by supersonic turbulence

Reference 53

Resolution
unresolved
no resolver link, observed 2026-07-13T02:50:38.049062Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-13T02:50:38.049062Z digest=sha256:5497eb7267fce4f89b8120d70a038fec84bbfbc2ba28603f059221327bf7eba2

Observation c63b7501-2f92-4b11-83e9-fc09a09621f0 · inbound

Accretion across scales: streamers, surface-layer transport, and rapid replenishment in young protoplanetary discs cites this paper.

Accretion across scales: streamers, surface-layer transport, and rapid replenishment in young protoplanetary discs Control of star formation by supersonic turbulence

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-04T11:34:03.303305Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:34:03.303305Z digest=sha256:6cd75bb55b520b03efde843901ab873aaa17b9c6797551253f843557845d8249