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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

Kinwah Wu ,
Mark Cropper  and
Gavin Ramsay
Kinwah Wu
Affiliation:
RCfTA, School of Physics University of Sydney, NSW 2006, Australia
Mark Cropper
Affiliation:
MSSL, University College London Holmbury St. Mary, Surrey, RH5 6NT, United Kingdom
Gavin Ramsay
Affiliation:
MSSL, University College London Holmbury St. Mary, Surrey, RH5 6NT, United Kingdom

Abstract

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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.

Type
Stellar Masses and Surface Gravities
Information
Symposium - International Astronomical Union , Volume 189: Fundamental Stellar Properties: The Interaction Between Observation and Theory , 1997 , pp. 115 - 118
Copyright
Copyright © Kluwer 1997 

References

Cropper, M., Ramsay, G. and Wu, K. (1997), MNRAS , in press.Google Scholar
Ishida, M. (1991), , , (ISAS RN 505).Google Scholar
Mewe, R., Kaastra, D.S. and Liedahl, D.A. (1995), Legacy (Journal of HEASARC) , 6, 16.Google Scholar
van Teeseling, A., Kaastra, J.S. and Heise, J. (1996), A&A , 312, 186.Google Scholar
Warner, B. (1996), Cataclysmic Variable Stars , Cambridge University Press.Google Scholar
Wu, K. Chanmugam, G. and Shaviv, G. (1994), ApJ , 426, 664.Google Scholar
Zdziarski, A.A. and Magdziarz, P. (1996), MNRAS , 279, 21.Google Scholar