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Paper Citation Record · LEDGER

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

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2410.07841.

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

pith.paper-citation-record.v1
2410.07841 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T21:56:45.210106Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T17:13:12.195368Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 4ef63a67-3665-48c6-9649-b8e9a1ef0c34 · inbound

Jets are the most robust observable ingredient of common envelope evolution cites this paper.

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

Resolution
unresolved
no resolver link, observed 2026-08-11T21:56:45.210106Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T21:56:45.210106Z digest=sha256:b892ff84978bd4fc8887d93a9b1a34d9d17a37f9cbc0e3f8c467c1521d46f4ac

Observation e0659250-1ec8-4ba5-a272-2a34607078a8 · inbound

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

Journey to the center of the common envelope evolution. Inner dynamics of the post-dynamical inspiral From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-11T21:31:37.325019Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T21:31:37.325019Z digest=sha256:f6a887204c81d18017c6887e42395afa40935054b754b703006662837073658d

Observation 543dbd69-1ad3-48b6-bdf4-55007b796023 · inbound

Mass-feeding of jet-launching white dwarfs in grazing and common envelope evolution cites this paper.

Mass-feeding of jet-launching white dwarfs in grazing and common envelope evolution From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral

Reference 103

Resolution
unresolved
no resolver link, observed 2026-08-07T13:10:30.730655Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:10:30.730655Z digest=sha256:afba21155429cf8ce644d0aff0df64bb71bb76b4175010ba6dfd57a9500296fd

Observation b8ba1e14-1edd-4997-b2f9-88b8268d1cb6 · inbound

The jet-feedback mechanism in common envelope evolution of planetary nebula progenitors cites this paper.

The jet-feedback mechanism in common envelope evolution of planetary nebula progenitors From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-07T06:09:41.933148Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T06:09:41.933148Z digest=sha256:8a4040f0351f660bd482876158525df1222784f769379248e38fceff2f468cc3

Observation e4c421ac-d32f-4017-a75d-76bbe7173edf · inbound

$\textit{BMAD}$-Circumbinary Magnetically Arrested Disks around Stellar or Black Hole Binaries: Hot Accretion Flows, Disk Properties, and Angular Momentum Transfer cites this paper.

$\textit{BMAD}$-Circumbinary Magnetically Arrested Disks around Stellar or Black Hole Binaries: Hot Accretion Flows, Disk Properties, and Angular Momentum Transfer From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral

Reference 187

Resolution
verified exact
local_arxiv, observed 2026-08-05T17:13:12.200740Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-08-05T17:13:12.072738Z digest=sha256:0afe488162c1efad39c8d65699676856ac310876d848a1301f470dfd9bcd7107