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TU Muscae and the Early-type Overcontact Binaries

Published online by Cambridge University Press:  12 April 2016

Dirk Terrell*
Affiliation:
Department of Space Studies, Southwest Research Institute, Boulder, CO 80301, USA

Abstract

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A simultaneous photometric and spectroscopic analysis of the purported early-type overcontact binary TU Muscae is presented. With a well-behaved light curve and a mass ratio far from unity, if TU Mus is indeed an overcontact system, it presents an interesting challenge for 3-D stellar evolution codes, like the Djehuty code, that will be applied to early-type overcontact binaries. The analysis shows TU Mus is slightly overcontact and that a detailed treatment of the reflection effect is important for modeling the light curves.

Type
Research Article
Copyright
Copyright © Astronomical Society of the Pacific 2002

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