Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-26T11:03:14.121Z Has data issue: false hasContentIssue false
  • English
  • Français

Feedback Mass Transfer in Cataclysmic Variables: An Explanation of the Behaviour of VY Scl Stars

Published online by Cambridge University Press:  25 April 2016

Kinwah Wu ,
Dayal T. Wickramasinghe  and
Brian Warner
Kinwah Wu
Affiliation:
Research Centre for Theoretical Astrophysics, School of Physics, University of Sydney, NSW 2006, Australia [email protected]
Dayal T. Wickramasinghe
Affiliation:
ANU Astrophysical Theory Centre and Department of Mathematics, SMS, Australian National University, Canberra, ACT 2601, Australia
Brian Warner
Affiliation:
Department of Astronomy, University of Cape Town, Rondebosch 7700, South Africa
Get access Rights & Permissions [Opens in a new window]

Abstract

We investigate irradiation-driven mass transfer in cataclysmic variables in the presence of shielding of the radiation by an accretion disk. We have shown that the shielding can cause a temporal drop of 3–5 magnitudes in the brightness of systems with orbital periods shorter than about 4 hr. This provides a possible explanation for the brightness variations in the VY Scl stars.

Keywords

starsbinariesclose — starsnovaecataclysmic variables — starswhite dwarfs
Type
Gallactic and Stellar
Information
Publications of the Astronomical Society of Australia , Volume 12 , Issue 1 , April 1995 , pp. 60 - 65
Copyright
Copyright © Astronomical Society of Australia 1995

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Faulkner, J. 1971, ApJ, 170, L9 Google Scholar
Hameury, J. M., King, A. R., & Lasota, J. P. 1986, A&A, 162, 71 Google Scholar
Harpaz, A., & Rappaport, S. 1991, ApJ, 383, 739 Google Scholar
Kovetz, A., Prialnik, D., & Shara, M. M. 1988, ApJ, 325, 828 Google Scholar
Livio, M., & Pringle, J. 1994, ApJ, 427, 956 Google Scholar
Osaki, Y. 1985, A&A, 144, 369 Google Scholar
Patterson, J. 1984, ApJS, 54, 443 Google Scholar
Podsiadlowski, Ph. 1991, Nature, 350, 136 CrossRefGoogle Scholar
Pringle, J. E. 1981, ARA&A, 19, 137 Google Scholar
Sarna, M. J. 1990, A&A, 239, 163 Google Scholar
Shafter, A. W. 1993, ApJ, 394, 268 Google Scholar
Verbunt, F., & Zwaan, C. 1981, A&A, 100, L7 Google Scholar
Warner, B. 1987, MNRAS, 227, 23 Google Scholar
Wu, K., Wickramasinghe, D. T., & Warner, B. 1995a, MNRAS, submittedGoogle Scholar
Wu, K., Wickramasinghe, D. T., & Warner, B. 1995b, ApJ, submittedGoogle Scholar