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Paper Citation Record · LEDGER

Jets are the most robust observable ingredient of common envelope evolution

As of 13 August 2026, this Paper Citation Record lists 21 of 21 outbound references and 1 inbound Pith citation observation for arXiv:2412.04017.

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

pith.paper-citation-record.v1
2412.04017 v2

Coverage vector

measured 21 of 21 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-11T21:56:45.217408Z

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measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T18:09:40.428855Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-11T18:09:45.243970Z

Reference resolution

21 of 21 outbound references displayed

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External citation measurements

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Outbound references

Observation 9ac41750-97c0-42f0-88c9-daa5ebf4c56c · outbound

This paper cites 2015, MNRAS, 453, 2115, doi: 10.1093/mnras/ stv1666 Akashi, M., & Soker, N.

Jets are the most robust observable ingredient of common envelope evolution 2015, MNRAS, 453, 2115, doi: 10.1093/mnras/ stv1666 Akashi, M., & Soker, N

Reference 1

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This paper cites Variability of Central Stars of Planetary Nebulae with the Zwicky Transient Facility. I. Methods, Short-Timescale Variables, Binary Candidates, and the Unusual Nucleus of WeSb 1.

Jets are the most robust observable ingredient of common envelope evolution Variability of Central Stars of Planetary Nebulae with the Zwicky Transient Facility. I. Methods, Short-Timescale Variables, Binary Candidates, and the Unusual Nucleus of WeSb 1

Reference 4

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Observation f5f19812-265e-46d3-81b5-6e046aa921a7 · outbound

This paper cites an unresolved cited work.

Jets are the most robust observable ingredient of common envelope evolution Unresolved cited work

Reference 5

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Observation 95eeead5-2405-4da3-931b-194952dd137a · outbound

This paper cites Journey to the center of the common envelope evolution. Inner dynamics of the post-dynamical inspiral.

Jets are the most robust observable ingredient of common envelope evolution Journey to the center of the common envelope evolution. Inner dynamics of the post-dynamical inspiral

Reference 7

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Observation 64b2a2f2-7f30-4ff0-8fed-01e625fe6c84 · outbound

This paper cites A., Cazzoli, S., Rechy-Garc ´ıa, J.

Jets are the most robust observable ingredient of common envelope evolution A., Cazzoli, S., Rechy-Garc ´ıa, J

Reference 8

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Observation f6548239-4983-4275-9c3e-7773afd2ca99 · outbound

This paper cites A., Imai, H., & Orosz, G.

Jets are the most robust observable ingredient of common envelope evolution A., Imai, H., & Orosz, G

Reference 10

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Observation 18fb58dd-16cd-4e8f-871d-1baeb11e5a33 · outbound

This paper cites 2020, MNRAS, 497, 3166, doi:.

Jets are the most robust observable ingredient of common envelope evolution 2020, MNRAS, 497, 3166, doi:

Reference 11

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Observation 00aa19ce-0965-48bd-9987-c3a05d7a843e · outbound

This paper cites Post-common-envelope planetary nebulae.

Jets are the most robust observable ingredient of common envelope evolution Post-common-envelope planetary nebulae

Reference 13

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Observation adf3dfd2-9655-409b-ae67-d27f26e053d8 · outbound

This paper cites 2010, MNRAS, 408, 2312, doi: 10.1111/j.1365-2966.

Jets are the most robust observable ingredient of common envelope evolution 2010, MNRAS, 408, 2312, doi: 10.1111/j.1365-2966

Reference 14

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Observation fb0d5cbe-ee97-4af2-8f11-f88b60c65d5a · outbound

This paper cites Successful Common Envelope Ejection and Binary Neutron Star Formation in 3D Hydrodynamics.

Jets are the most robust observable ingredient of common envelope evolution Successful Common Envelope Ejection and Binary Neutron Star Formation in 3D Hydrodynamics

Reference 15

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Observation 9bd6ef99-1159-42fa-8bb4-3608a0d01af8 · outbound

This paper cites Halving spaces and lower bounds in real enumerative geometry.

Jets are the most robust observable ingredient of common envelope evolution Halving spaces and lower bounds in real enumerative geometry

Reference 16

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Observation 0c46d5a2-661c-42c7-a55a-6f104ec3aa12 · outbound

This paper cites A., Redman, M.

Jets are the most robust observable ingredient of common envelope evolution A., Redman, M

Reference 17

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Observation ca24aea3-e3ea-4960-8457-6f72de147f90 · outbound

This paper cites The Evolution of Binaries Embedded Within Common Envelopes.

Jets are the most robust observable ingredient of common envelope evolution The Evolution of Binaries Embedded Within Common Envelopes

Reference 19

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Observation 72da642d-ba85-4424-9d97-40fd7cfbdb51 · outbound

This paper cites High-Speed Outflows and Dusty Disks during the AGB to PN Transition: The PANORAMA survey.

Jets are the most robust observable ingredient of common envelope evolution High-Speed Outflows and Dusty Disks during the AGB to PN Transition: The PANORAMA survey

Reference 20

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Observation 4ef63a67-3665-48c6-9649-b8e9a1ef0c34 · outbound

This paper cites From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral.

Jets are the most robust observable ingredient of common envelope evolution From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral

Reference 21

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Observation 4533f4a3-b6f4-412b-9094-b0f685084117 · outbound

This paper cites C., & Nordhaus, J.

Jets are the most robust observable ingredient of common envelope evolution C., & Nordhaus, J

Reference 22

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This paper cites 2020, MNRAS, 497, 2855, doi: 10.1093/mnras/staa2145.

Jets are the most robust observable ingredient of common envelope evolution 2020, MNRAS, 497, 2855, doi: 10.1093/mnras/staa2145

Reference 23

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Observation 5e865699-bc5d-4e22-bf59-156ae2ed2210 · outbound

This paper cites 2024, MNRAS, 532, 692, doi:10.

Jets are the most robust observable ingredient of common envelope evolution 2024, MNRAS, 532, 692, doi:10

Reference 96

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Observation fb6344df-bb93-4af3-bf28-b3491434fc83 · outbound

This paper cites C., Frew, D.

Jets are the most robust observable ingredient of common envelope evolution C., Frew, D

Reference 319

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Observation dea8dc95-ee35-4693-a91e-4651e9a39e56 · outbound

This paper cites On the response of massive main sequence stars to mass accretion and outflow at high rates.

Jets are the most robust observable ingredient of common envelope evolution On the response of massive main sequence stars to mass accretion and outflow at high rates

Reference 778

Resolution
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Observation 60de5c3d-8480-4d11-96cf-682486b2e6cd · outbound

This paper cites 2024, MNRAS, 530, 3327, doi: 10.1093/mnras/stae1013 Estrella-Trujillo, D., Hern ´andez-Mart´ınez, L., Vel ´azquez, P.

Jets are the most robust observable ingredient of common envelope evolution 2024, MNRAS, 530, 3327, doi: 10.1093/mnras/stae1013 Estrella-Trujillo, D., Hern ´andez-Mart´ınez, L., Vel ´azquez, P

Reference 2277

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Pith citing papers

Observation 60e96441-16ff-4fd1-a9ab-3b30cb1957da · inbound

Hyperaccreting Magnetised Neutron Stars inside Rotating Massive Envelopes: Low-Power Jets and Precursor Flares cites this paper.

Hyperaccreting Magnetised Neutron Stars inside Rotating Massive Envelopes: Low-Power Jets and Precursor Flares Jets are the most robust observable ingredient of common envelope evolution

Reference 24

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