Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-29T09:37:22.515Z Has data issue: false hasContentIssue false
  • English
  • Français

Thermal-Tidal Instability Model of Dwarf Novae Below the Period Gap: A Unification Theory

Published online by Cambridge University Press:  12 April 2016

Y. Osaki
Y. Osaki*
Affiliation:
Department of Astronomy, School of Science, University of Tokyo, Bunkyo-ku, Tokyo, 113, Japan

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 unification theory is proposed in which almost all of outburst behavior in dwarf novae may be understood in a unified way within the basic framework of the disk instability model. In particular, a rich variety of outburst behavior of cataclysmic variables below the period gap may be understood by the thermal-tidal instability model in which the coupling of the two intrinsic instabilities in the accretion disk plays a unique role.

Type
Accretion Discs
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 127 - 130
Copyright
Copyright © Kluwer 1996

References

Hirose, M., Osaki, Y., 1990, PASJ, 42, 135 Google Scholar
Kato, T., Kurijaya, C., 1995, PASJ, 47, 163 Google Scholar
Lubow, S.H., 1991, Ap. J., 381, 259 CrossRefGoogle Scholar
Osaki, Y., 1989, PASJ, 41, 1005 Google Scholar
Osaki, Y., 1995a, PASJ, 47, 47 Google Scholar
Osaki, Y., 1995b, PASJ, 47, L1l Google Scholar
Osaki, Y., 1995c, PASJ, 47, L25 Google Scholar
Osaki, Y. 1995d, in “Cataclysmic Variables”, eds Bianchini, A. et al., Kluwer, p 307 CrossRefGoogle Scholar
Robertson, J.W., Honeycutt, R.K., Turner, G.W. 1995, PASP, 107, 443 Google Scholar
Skillman, D.R., Patterson, J., 1993, Ap. J., 417, 298 Google Scholar
Vogt, N., 1993, in “Cataclysmic Variables and Related Physics”, eds Regev, O., Shaviv, G., Ann. Israel Phys. Soc., 10, 63 Google Scholar
Whitehurst, R., 1988, MNRAS, 232, 35 Google Scholar