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Paper Citation Record · LEDGER

Control of star formation by supersonic turbulence

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 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 12 of 12 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 12 of 12 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:44:36.770920Z

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

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  • 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 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:61c60cb5f622b9bbfd4ed2cb66e6c2bda576d304305bfce13042abbd771d2235

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 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:54b070516a3607eaf1d9bf4e7773648019b9daf72bef1748f357c1766ba40fad

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 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d46a90a272c1136d565ce145b493b66bfcfcb0e204f981cd707113eb3892eb3d

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 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:e74e9ee1c72eef194389c359c8529570bfae0177e93ff769011f3253bd9c005b

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 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:5f2a8aa5198bdd8e85fbef972b05b600602d2622fced8afea770c7fcdf32221a

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=sha256:02b98f328f6bd5c3319bab52a7a9c306e94820d86aea97f0694ab0f29665bb9b

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=sha256:11872d6ae62a4850211bb78ee577dae2406916aec49b25e7a5ee1c5e0a2998af

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 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:101d8b666679313bd3b5682ca67d73ff04f96d5cc2db61aeb94df32fd2519861

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=sha256:72966cfeebaaed5c20f0bfb32410bdbd7f59fb4430c6e08ca1a747551b044ec4

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=sha256:20a0081b68974e0e39074ae8c2b57d7c4bb2a3291e6b62408ce540b7a80419d0

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:effd320c078bd660528143e610f7a191d16043cc8f673768742dc53d93c0b3fd

Observation 01a4199d-6d54-420f-8ec0-00f95848eacf · inbound

The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae cites this paper.

The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae Control of star formation by supersonic turbulence

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-14T04:44:36.770920Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:44:36.770920Z digest=sha256:c4c3729f5ef99e7f3cb759f55c430680ad13c93956d836968c76f32ed4c3db5c