Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-12-01T02:42:52.994Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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