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Cataclysmic Variable Stars - How and Why They Vary

Name: Cataclysmic Variable Stars - How and Why They Vary
Author: Coel Hellier
ISBN: 9781852332112

by Coel Hellier

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Overview

... dwarf must be below the Chandrasekhar limit of ≈ 1.4 M ( see Section 2.1 ) the red dwarf must be also . The size of ... braking decreases the binary separation , over hundreds of millions of years , until the Roche lobe makes ...

Synopsis

This text presents numerous illustrations of the observed variability of cataclysmic variable stars. It provides a clear explanation and thorough up-to-date overview of this phenomena at a level accessible to the advanced amateur or undergraduate student.

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Book Details

Published

February 23, 2001

Publisher

Springer Science & Business Media

Pages

232

ISBN

9781852332112