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arXiv · 1404.0591

Absolute Properties of the Eclipsing Binary Star AP Andromedae

Claud H. Sandberg Lacy·Guillermo Torres·Francis C. Fekel·Matthew W. Muterspaugh
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Abstract

AP And is a well-detached F5 eclipsing binary star for which only a very limited amount of information was available before this publication. We have obtained very extensive measurements of the light curve (19097 differential V magnitude observations) and a radial velocity curve (83 spectroscopic observations) which allow us to fit orbits and determine the absolute properties of the components very accurately: masses of 1.277 +/- 0.004 and 1.251 +/- 0.004 solar masses, radii of 1.233 +/- 0.006 and 1.1953 +/- 0.005 solar radii, and temperatures of 6565 +/- 150 K and 6495 +/- 150 K. The distance to the system is about 400 +/- 30 pc. Comparison with the theoretical properties of the stellar evolutionary models of the Yonsei-Yale series of Yi et al. shows good agreement between the observations and the theory at an age of about 500 Myr and a slightly sub-solar metallicity.

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Claud H. Sandberg Lacy, Guillermo Torres, Francis C. Fekel, Matthew W. Muterspaugh. 2014-04-02. Absolute Properties of the Eclipsing Binary Star AP Andromedae. https://doi.org/10.1088/0004-6256%2F147%2F6%2F148

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