Pith sign in

REVIEW 1 cited by

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2107.10765 v1 pith:Y75M4TFV submitted 2021-07-22 astro-ph.SR

Analysis of apsidal motion in eclipsing binaries using TESS data II. A test of internal stellar structure}

A. Claret , A. Gim\'enez , D. Baroch , I. Ribas , J.C. Morales , G. Anglada-Escud\'e This is my paper
classification astro-ph.SR
keywords apsidalbinariescomparisoneclipsinginternalmotionparametersprecise
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

We have determined the apsidal motion rate of 27 double-lined eclipsing binaries with precise physical parameters. The obtained values, corrected for their relativistic contribution, yield precise empirical parameters of the internal stellar density concentration. The comparison of these results with the predictions based on new theoretical models shows very good agreement. Small deviations are identified but remain within the observational uncertainties and the path for a refined comparison is indicated.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Self-Interacting Dark Matter in Brown Dwarfs

    astro-ph.SR 2026-05 unverdicted novelty 3.0

    Brown dwarfs modeled with a self-interacting dark matter fluid component show modified radii and second-order Love numbers due to core accumulation.