Orbital and physical parameters of eclipsing binaries from the All-Sky Automated Survey catalogue

2014/05/12 by K. G. Hełminiak, R. Brahm, Rafael Brahm +7
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Astrophysics and Star Formation Studies #Binary number #Binary star #Orbital elements #Physics #Sky #Stars #Stellar, planetary, and galactic studies #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201220985

published as A&A 567, A64 (2014) · 9 pages, 11 figures, 3 tables, accpeted for publication in A&A

arxiv created 2014/05/12 · openalex publication_date 2014/06/05 · arxiv updated 2014/09/05 · openalex created_date 2022/10/02 · openalex updated_date 2026/08/01

Abstract

Aims. We present the results of the combined photometric and spectroscopic analysis of a bright (V = 9.14), close (d = 31 pc), late-type detached eclipsing binary, AK Fornacis. This P = 3.981 d system has not been previously recognised as a double-lined spectroscopic binary, and this is the first full physical model of this unique target.

Citations

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