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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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
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