Pith. sign in

Paper Citation Record · LEDGER

Stellar evolution of low and intermediate-mass stars. IV. Hydrodynamically-based overshoot and nucleosynthesis in AGB stars

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9706122.

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

pith.paper-citation-record.v1
astro-ph/9706122 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 2026-08-08T06:32:00.761636+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T14:56:13.197555Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-25T02:55:16.277216Z

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 d1e0241b-48a8-4ecf-9fe5-cb461659cec0 · inbound

Evolution and final fates of massive stars cites this paper.

Evolution and final fates of massive stars Stellar evolution of low and intermediate-mass stars. IV. Hydrodynamically-based overshoot and nucleosynthesis in AGB stars

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-08T14:56:13.197555Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T14:56:13.197555Z digest=sha256:b9c5ad79a38f0854ea20c9c4b3af20d09c9afa8ff266e3330fc70063e5d50829

Observation d0408e92-fe74-48ad-92d5-b17cad801b03 · inbound

The s- and r- components of the proto-solar composition cites this paper.

The s- and r- components of the proto-solar composition Stellar evolution of low and intermediate-mass stars. IV. Hydrodynamically-based overshoot and nucleosynthesis in AGB stars

Reference 23

Resolution
verified exact
local_arxiv, observed 2026-05-25T02:55:16.279753Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-05-25T02:54:57.383230Z digest=sha256:9dded99db6c26570054d6693bfc6324ba5359a01c10f28851983151613b071f1