Absolute dimensions of eclipsing binaries

2006/10/13 by John Southworth, J. Southworth, J. V. Clausen · 4 citations
Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Binary star #Biology #Cluster (spacecraft) #Context (archaeology) #Physics #Star cluster #Stars #Stellar evolution #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065614

19 pages, 9 figures, accepted for publication by A&A

arxiv created 2006/10/13 · openalex publication_date 2006/10/16 · arxiv updated 2009/12/01 · openalex created_date 2022/10/03 · openalex updated_date 2026/07/31

Abstract

Context.The study of detached eclipsing binaries which are members of stellar clusters is is a powerful way of determining the properties of the cluster and of constraining the physical ingredients of theoretical stellar evolutionary models.

Citations

• The Shortest-Period M-Dwarf Eclipsing System BW3 V38
• Absolute Dimensions of the M‐Type Eclipsing Binary YY Geminorum (Castor C): A Challenge to Evolutionary Models in the Lower Main Sequence
• Transformations from Theoretical Hertzsprung-Russell Diagrams to Color-Magnitude Diagrams: Effective Temperatures, B-V Colors, and Bolometric Corrections
• Eclipsing binaries in open clusters - II. V453 Cyg in NGC 6871

Cited by

• Absolute Dimensions and Apsidal Motion of the Young Detached System LT Canis Majoris
• Absolute dimensions of detached eclipsing binaries - II. The metallic-lined system XY Ceti
• Homogeneous studies of transiting extrasolar planets – I. Light-curve analyses
• Chemical evolution of high-mass stars in close binaries - I. The eclipsing binary V453 Cygni