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Determining the masses of white dwarfs in magnetic cataclysmic variables from x-ray observations
Published online by Cambridge University Press: 25 May 2016
Abstract
A method to determine the masses of white dwarfs in magnetic cataclysmic variables from X-ray observations is presented. The method is appropriate for both eclipsing and non-eclipsing systems, for it is insensitive to the orbital inclination of the systems.
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- Stellar Masses and Surface Gravities
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- Copyright © Kluwer 1997