Accurate fundamental parameters of eclipsing binary stars

Southworth, John; Smalley, Barry; Maxted, Pierre; Etzel, P.B.

Abstract

The study of detached eclipsing binaries is one of the most powerful ways to investigate the properties of individual stars and stellar systems. We present preliminary masses, radii and effective temperatures for the eclipsing binary WW Aurigae, which is composed of two metallic-lined A-type stars. We also reanalyse the data on HD 23642, an A-type eclipsing binary member of the Pleiades open cluster with a metallic-lined component, and determine its distance to be 139 +/- 4 pc. This is in agreement with the traditional Pleiades distance, but in disagreement with distance to the Pleiades, and to HD 23642 itself, derived from Hipparcos trigonometrical parallaxes.

Citation

Southworth, J., Smalley, B., Maxted, P., & Etzel, P. (2004). Accurate fundamental parameters of eclipsing binary stars. Proceedings of the International Astronomical Union, 2004(IAUS224), 548-561. https://doi.org/10.1017/S1743921305009324

• Journal Article Type: Article
• Online Publication Date: Mar 2, 2005
• Publication Date: 2004-07
• Publicly Available Date: May 26, 2023
• Journal: Proceedings of the International Astronomical Union
• Print ISSN: 1743-9213
• Publisher: Cambridge University Press
• Peer Reviewed: Peer Reviewed
• Volume: 2004
• Issue: IAUS224
• Pages: 548-561
• DOI: https://doi.org/10.1017/S1743921305009324
• Keywords: Astrophysics
• Publisher URL: http://dx.doi.org/10.1017/S1743921305009324