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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 23 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 2026-08-22T06:32:14.747728+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

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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=sha256:58856c57d8df3acdaeb50d192bcc8f19174322b9c30fe06147f2f188b09b4d63

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=sha256:2586743e69dc3d53e6e718153ae7859195b393f776668aa1db4bbe2817282406

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=sha256:42e7e3859728a482126554420d9556b219456ef928a9fc017ff363c0ec7715a0

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=sha256:250704f9743356e3e9d2df4fa49a747b1d0955df8c994dab8776e92cd89fdb88

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 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-08-05T17:13:12.072738Z digest=sha256:ca662fbaf1f2440f91ed83981a21b7ccc3aa3b776429d7b36ff06ac6aa25dc78