Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Close binary evolution I. The tidally induced shear mixing in rotating binaries
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1306.6731.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T13:33:06.503714Z
A source-named dated measurement, never combined with another source.
Source: cited_works
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 852ebdf4-38c8-4122-8fc0-3430aa4ec79d · inbound
The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants cites this paper.
The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants Close binary evolution I. The tidally induced shear mixing in rotating binaries
Reference 287
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T02:41:03.814429Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 790a0f4f-6315-499a-9d9b-386647cd0609 · inbound
The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars cites this paper.
The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars Close binary evolution I. The tidally induced shear mixing in rotating binaries
Reference 82
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T13:33:06.503714Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.