Paper Citation Record · LEDGER

Are passive protostellar disks stable to self-shadowing?

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0007399.

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

pith.paper-citation-record.v1
astro-ph/0007399 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T02:12:06.800442Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

0
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation ed786eaa-e419-4bbd-a572-9686cec79b3e · inbound

Planet formation at the inner edge of the dead zone II. Outbursts, rings, vortices, and suppression of planetesimal formation cites this paper.

Planet formation at the inner edge of the dead zone II. Outbursts, rings, vortices, and suppression of planetesimal formation Are passive protostellar disks stable to self-shadowing?

Reference 262

Resolution: verified exact; local_arxiv, observed 2026-06-27T11:40:53.509434Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 809f018a-c9fd-40d6-95d0-bb1a21cd82d1 · inbound

The Influence of Dust Composition on Accretion Outbursts cites this paper.

The Influence of Dust Composition on Accretion Outbursts Are passive protostellar disks stable to self-shadowing?

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-01T02:12:06.800442Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.