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Paper Citation Record · LEDGER

Revisiting gravitational instability in protostellar discs with improved radiative cooling models

As of 16 August 2026, this Paper Citation Record lists 86 of 86 outbound references and 0 inbound Pith citation observations for arXiv:2608.13058.

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

pith.paper-citation-record.v1
2608.13058 v1

Coverage vector

measured 86 of 86 reference resolution

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measured 86 of 86 standing notices

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Pith citing papers itemized under the disclosed page cap.

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measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

86 of 86 outbound references displayed

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External citation measurements

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Outbound references

Observation 7e75d30f-7d17-45f1-8654-b5db113681af · outbound

This paper cites arXiv , author =:2510.19915 , journal =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models arXiv , author =:2510.19915 , journal =

Reference 1

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Observation 2c480780-c21f-4e14-b217-abd4227ef49c · outbound

This paper cites doi:10.1093/mnras/stab2657 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/stab2657 , eprint =

Reference 5

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Observation b16084d7-bd0f-4045-8c70-82e11dad2888 · outbound

This paper cites Early Planet Formation in Embedded Disks (eDisk) XIV: Flared Dust Distribution and Viscous Accretion Heating of the Disk around R CrA IRS 7B-a.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models Early Planet Formation in Embedded Disks (eDisk) XIV: Flared Dust Distribution and Viscous Accretion Heating of the Disk around R CrA IRS 7B-a

Reference 6

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Observation fa946465-0003-4b0b-8fd5-282269fd0e8c · outbound

This paper cites Temperature structures of embedded disks: young disks in Taurus are warm.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models Temperature structures of embedded disks: young disks in Taurus are warm

Reference 7

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Observation b780158e-cd3c-4ddd-aefd-ad3bdb533632 · outbound

This paper cites A low-mass protostar's disk-envelope interface: disk-shadowing evidence from ALMA DCO+ observations of VLA1623.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models A low-mass protostar's disk-envelope interface: disk-shadowing evidence from ALMA DCO+ observations of VLA1623

Reference 8

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Observation fae13046-faab-4b32-8918-a44d834859d6 · outbound

This paper cites Unveiling the physical conditions of the youngest disks: A warm embedded disk in L1527.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models Unveiling the physical conditions of the youngest disks: A warm embedded disk in L1527

Reference 9

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Observation 0de51880-cd24-4cc5-aec1-d2d52fdbf765 · outbound

This paper cites Global Simulations of Gravitational Instability in Protostellar Disks with Full Radiation Transport II. Locality of Gravitoturbulence, Clumpy Spirals, and Implications for Observable Substructure.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models Global Simulations of Gravitational Instability in Protostellar Disks with Full Radiation Transport II. Locality of Gravitoturbulence, Clumpy Spirals, and Implications for Observable Substructure

Reference 10

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Observation 30120ee5-2447-4ab8-a8c8-2d21d5cef980 · outbound

This paper cites On the gravitational stability of gravito-turbulent accretion disks.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models On the gravitational stability of gravito-turbulent accretion disks

Reference 11

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Observation fe22c719-555e-4d6a-9827-d4530a79e1a7 · outbound

This paper cites doi:10.1038/s41550-020-01297-6 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1038/s41550-020-01297-6 , eprint =

Reference 13

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Observation 5d01a4ce-d1a7-416e-969f-6cdf76a38eab · outbound

This paper cites doi:10.1093/mnras/stv2128 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/stv2128 , eprint =

Reference 14

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Observation 41843a2f-2465-45c9-8f8b-61ced2429068 · outbound

This paper cites doi:10.1086/430813 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1086/430813 , eprint =

Reference 15

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models Unresolved cited work

Reference 17

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models Unresolved cited work

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models Unresolved cited work

Reference 19

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Observation 27154c04-82e1-4324-934e-af9d4a9c8e41 · outbound

This paper cites doi:10.1093/mnras/stv970 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/stv970 , eprint =

Reference 20

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Observation 128e149b-74c0-4a94-a0df-1fb6817fc22f · outbound

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/staa2596 , eprint =

Reference 21

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models Unresolved cited work

Reference 22

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Observation be1e4879-54da-486d-8733-9ee269c0f247 · outbound

This paper cites doi:10.1093/mnrasl/slaf096 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnrasl/slaf096 , eprint =

Reference 23

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Observation 24695e06-ee49-4c21-9cff-e6972eb8526f · outbound

This paper cites arXiv , author =:2510.02437 , journal =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models arXiv , author =:2510.02437 , journal =

Reference 24

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Observation f6643657-6d39-4b95-b1a7-eb198dbb8f31 · outbound

This paper cites On Gas-Drag Induced Rapid Migration of Solids in a Non-Uniform Solar Nebula.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models On Gas-Drag Induced Rapid Migration of Solids in a Non-Uniform Solar Nebula

Reference 25

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Observation b54af370-9255-40bc-9506-3489d4caf6c8 · outbound

This paper cites The temporal requirements of directly observing self-gravitating spiral waves in protoplanetary discs with ALMA.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models The temporal requirements of directly observing self-gravitating spiral waves in protoplanetary discs with ALMA

Reference 26

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1086/428899 , eprint =

Reference 27

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1086/421288 , eprint =

Reference 28

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models Unresolved cited work

Reference 29

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/stae167 , eprint =

Reference 30

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Observation d3f4cf2c-84ff-4d26-bb4f-05525e81a8db · outbound

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models Observational appearance

Reference 31

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This paper cites Continuing to Hide Signatures of Gravitational Instability in Protoplanetary Discs with Planets.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models Continuing to Hide Signatures of Gravitational Instability in Protoplanetary Discs with Planets

Reference 32

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models Blobs, spiral arms, and a possible planet around HD 169142

Reference 34

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1038/s41550-022-01634-x , eprint =

Reference 35

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models Unresolved cited work

Reference 36

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models arXiv , author =:2512.00498 , journal =

Reference 37

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models arXiv , author =:2512.02237 , journal =

Reference 38

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1086/304869 , eprint =

Reference 39

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models Harris and K

Reference 40

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1071/AS07022 , eprint =

Reference 41

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/stz2215 , eprint =

Reference 42

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Observation 0fd74fd1-ec66-4a30-a2fb-9695349d30d2 · outbound

This paper cites doi:10.1038/s41550-025-02552-4 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1038/s41550-025-02552-4 , eprint =

Reference 43

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Observation deece7df-bf0c-48be-a0a5-1400d98112b9 · outbound

This paper cites doi:10.1093/mnras/sty169 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/sty169 , eprint =

Reference 44

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Observation a57a9f71-5b2e-414a-a930-8bec51a000d0 · outbound

This paper cites doi:10.1086/524101 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1086/524101 , eprint =

Reference 46

Resolution
verified exact
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation b7e4525b-39c3-40e6-a666-c6fc773c5cc2 · outbound

This paper cites doi:10.1093/mnras/stx2870 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/stx2870 , eprint =

Reference 47

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Observation ad289905-a42f-43a5-a711-44c36fb8c2d8 · outbound

This paper cites doi:10.1093/mnras/stt032 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/stt032 , eprint =

Reference 48

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Observation 9e9917e2-5f4e-46c8-b5dd-7972e41654f5 · outbound

This paper cites doi:10.1051/0004-6361:20065806 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1051/0004-6361:20065806 , eprint =

Reference 49

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Observation 7bf3b951-e67b-4c3c-ae12-1931ff56d5bd · outbound

This paper cites The formation of brown dwarfs and low-mass stars by disc fragmentation.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models The formation of brown dwarfs and low-mass stars by disc fragmentation

Reference 51

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation 9e61a9ac-4628-4e8e-bae0-10cb939e0a17 · outbound

This paper cites doi:10.1111/j.1365-2966.2005.08875.x , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1111/j.1365-2966.2005.08875.x , eprint =

Reference 53

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Observation e0a13a88-ce81-462d-9d39-a2eee640a18a · outbound

This paper cites doi:10.1093/mnras/stv1997 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/stv1997 , eprint =

Reference 54

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Observation 77b228d6-bc20-44ae-9cfc-5f7a2cfb04a3 · outbound

This paper cites The evolution of self-gravitating accretion discs.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models The evolution of self-gravitating accretion discs

Reference 55

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation fc6ac58c-78aa-447e-af9c-e4212f74e898 · outbound

This paper cites arXiv , author =:2510.19635 , journal =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models arXiv , author =:2510.19635 , journal =

Reference 56

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Source-reported events for the cited work

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Observation be56f9ea-7556-468a-8a45-a3189fad524d · outbound

This paper cites an unresolved cited work.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models Unresolved cited work

Reference 57

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Observation d93203a8-1bc7-4c27-84b2-61bda17b0ae7 · outbound

This paper cites doi:10.1051/0004-6361/200912325 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1051/0004-6361/200912325 , eprint =

Reference 58

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Observation 40e5b6d3-e851-456f-99b6-4d528c1cd170 · outbound

This paper cites doi:10.1146/annurev-astro-081710-102548 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1146/annurev-astro-081710-102548 , eprint =

Reference 59

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Observation 70148893-1b96-4b2b-8844-b41bbe3dd692 · outbound

This paper cites doi:10.1093/mnras/staf1018 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/staf1018 , eprint =

Reference 60

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Observation 2fe616fa-f29b-4505-ad39-6d5556b893c7 · outbound

This paper cites doi:10.1093/mnras/staf644 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/staf644 , eprint =

Reference 61

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Observation d0aabb19-726b-4629-b21c-8644feef743b · outbound

This paper cites doi:10.1093/mnrasl/slad027 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnrasl/slad027 , eprint =

Reference 62

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Observation b47ffb4f-c472-42f4-a0ba-bc7f7a5e37d7 · outbound

This paper cites doi:10.1093/mnras/stae2167 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/stae2167 , eprint =

Reference 63

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Observation d8abb631-d72c-4f68-8cc7-caf464b7a40d · outbound

This paper cites doi:10.1093/mnras/staf714 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/staf714 , eprint =

Reference 65

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verified exact
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation dab40ea1-19f3-49dd-8a5c-c57e1c463fca · outbound

This paper cites doi:10.1093/mnras/staf743 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/staf743 , eprint =

Reference 66

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unresolved
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Source-reported events for the cited work

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Observation 5cf172fb-67ad-44a2-bd9c-f3afa6f09e3a · outbound

This paper cites doi:10.1093/mnras/staa1590 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/staa1590 , eprint =

Reference 67

Resolution
verified exact
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation 5fd8ebf7-2284-4683-8f21-dca65221e55c · outbound

This paper cites doi:10.1111/j.1365-2966.2008.14373.x , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1111/j.1365-2966.2008.14373.x , eprint =

Reference 68

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Observation 085a2c8d-558f-461d-b179-01f6c9423d9a · outbound

This paper cites Planet formation around M dwarfs via disc instability: Fragmentation conditions and protoplanet properties.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models Planet formation around M dwarfs via disc instability: Fragmentation conditions and protoplanet properties

Reference 69

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation e1fafe73-1094-488a-ae25-031296241063 · outbound

This paper cites MESA Isochrones and Stellar Tracks (MIST) 0: Methods for the construction of stellar isochrones.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models MESA Isochrones and Stellar Tracks (MIST) 0: Methods for the construction of stellar isochrones

Reference 70

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Observation fdb5b605-8d3e-452a-81b9-15babefa185b · outbound

This paper cites an unresolved cited work.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models Unresolved cited work

Reference 71

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Observation f404a6d3-dd77-4a28-b2e0-0d94adab8960 · outbound

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1111/j.1365-2966.2010.17158.x , eprint =

Reference 72

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Observation 42b7eaff-f10a-483d-8ed3-5980fd60308a · outbound

This paper cites doi:10.1017/pasa.2018.25 , eid =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1017/pasa.2018.25 , eid =

Reference 73

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Observation 337ba56f-296f-4ee8-a431-743dff3e217e · outbound

This paper cites MESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models MESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models

Reference 74

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Observation df8c74c1-cc54-4a4b-a908-aa80dac7a5f8 · outbound

This paper cites doi:10.1093/mnras/staa883 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/staa883 , eprint =

Reference 75

Resolution
unresolved
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Observation 6bc217ac-bc27-47f0-abfd-80519aac3208 · outbound

This paper cites Fragment Production and Survival in Irradiated Disks: A Comprehensive Cooling Criterion.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models Fragment Production and Survival in Irradiated Disks: A Comprehensive Cooling Criterion

Reference 76

Resolution
unresolved
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Unavailable: canonical work link unavailable.

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Observation b8004a68-ec96-42f7-9c2e-e8174425e4ac · outbound

This paper cites doi:10.1088/0004-637X/710/2/1375 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1088/0004-637X/710/2/1375 , eprint =

Reference 77

Resolution
unresolved
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Observation f48a0094-2e98-4b95-ba0f-650a1a205717 · outbound

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1111/j.1365-2966.2012.22035.x , eprint =

Reference 78

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unresolved
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Observation b40d80aa-aa7a-496c-b9d4-320653452345 · outbound

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1111/j.1365-2966.2011.18344.x , eprint =

Reference 79

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unresolved
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Observation 6fa1811a-32e5-4775-859b-f61ded84600a · outbound

This paper cites doi:10.1111/j.1365-2966.2006.11119.x , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1111/j.1365-2966.2006.11119.x , eprint =

Reference 80

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 740a97c7-7711-4fb2-a270-65c6a3db3b7c · outbound

This paper cites doi:10.1088/0004-637X/704/1/281 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1088/0004-637X/704/1/281 , eprint =

Reference 81

Resolution
verified exact
doi, observed 2026-08-15T17:46:03.855375Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation 1331e497-21cf-4d7e-b3b9-72bed0d05366 · outbound

This paper cites doi:10.1111/j.1365-2966.2009.14774.x , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1111/j.1365-2966.2009.14774.x , eprint =

Reference 82

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Observation 5179575c-e4a4-4041-a7bb-2228eb4cdd6d · outbound

This paper cites doi:10.1093/mnras/stae1249 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/stae1249 , eprint =

Reference 83

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Observation 6d760ffe-8eab-49cd-97be-197f12904dc2 · outbound

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1146/annurev-astro-081915-023307 , eprint =

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Observation e8726f92-e015-41fa-a4fc-03efde3b2f7e · outbound

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models Unresolved cited work

Reference 85

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/sty1290 , eprint =

Reference 86

Resolution
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Observation 8fe84739-0730-4157-8aec-4ead640bf51b · outbound

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/stu2432 , eprint =

Reference 87

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1051/0004-6361:20077373 , eprint =

Reference 88

Resolution
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Source-reported events for the cited work

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Observation 544b7e3c-ee41-48f2-94b4-0ec79438cfbd · outbound

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1086/320631 , eprint =

Reference 89

Resolution
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This paper cites The role of the drag force in the gravitational stability of dusty planet forming disc -- I. Analytical theory.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models The role of the drag force in the gravitational stability of dusty planet forming disc -- I. Analytical theory

Reference 90

Resolution
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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1111/j.1365-2966.2004.08339.x , eprint =

Reference 91

Resolution
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Unavailable: canonical work link unavailable.

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Observation 1465d79e-5fb0-4d44-9dca-ec633d756d49 · outbound

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1111/j.1745-3933.2006.00215.x , eprint =

Reference 92

Resolution
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Unavailable: canonical work link unavailable.

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Observation 12c5879c-4ba8-44f7-bfd7-1b9ab72de362 · outbound

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models Unresolved cited work

Reference 93

Resolution
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Unavailable: canonical work link unavailable.

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1038/s41586-020-2779-6 , eprint =

Reference 94

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/sty593 , eprint =

Reference 95

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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This paper cites doi:10.1093/mnras/staa187 , eprint =.

Revisiting gravitational instability in protostellar discs with improved radiative cooling models doi:10.1093/mnras/staa187 , eprint =

Reference 96

Resolution
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Pith citing papers

No inbound Pith citation observations are available.