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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 298))

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Abstract

With the advent of modern surveys which yield more M-type eclipsing binary stars and with a new light curve analysis code which incorporates atmospheric models for cool stars, the time is right for a renaissance in understanding the lower main sequence.

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© 2003 Springer Science+Business Media Dordrecht

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Shaw, J.S. (2003). Very Cool Close Binary Systems. In: Cheng, K.S., Leung, K.C., Li, T.P. (eds) Stellar Astrophysics — A Tribute to Helmut A. Abt. Astrophysics and Space Science Library, vol 298. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-0403-8_13

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  • DOI: https://doi.org/10.1007/978-94-017-0403-8_13

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-6452-3

  • Online ISBN: 978-94-017-0403-8

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