Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-30T22:11:48.128Z Has data issue: false hasContentIssue false
  • English
  • Français

The Implications of Disc Instabilities on Cataclysmic Variable Structure and Evolution

Published online by Cambridge University Press:  22 February 2018

J.-P. Lasota
J.-P. Lasota*
Affiliation:
Institut d'Astrophysique de Paris, France

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.

Applications of the thermal-viscous disc instability model to various classes of cataclysmic variable very often require the accretion disc to be truncated. I argue that in most cases this inner truncation must be due to the white dwarf's magnetic field.

Resumen

Resumen

Al aplicar el modelo de inestabilidad ténnieo-viscosa del disco a varias clases de variables catacíismicas, con frecuencia se requiere que el disco de aereción sea truncado. Arguyo que en la mayoría de los casos este truncamiento interno se debe al campo magnético de la enana blanca.

Keywords

AccretionAccretion Discs — Instabilities — NovaeCataclysmic Variables — Stars: Evolution
Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 124 - 127
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

Buckley, D. A. H., Sekiguchi, K., Motch, C. et al. 1995, MNRAS, 275, 1028 Google Scholar
Cheng, F. H., Sion, E. M., Szkody, P., & Huang, M. 1997, ApJL, 484, L149 Google Scholar
Dubus, G., Hameury, J.-M., & Lasota, J.-P. 2001, A&A, 373, 251 Google Scholar
Honeycutt, R.K., Robertson, J.W., 1998, AJ, 116, 1961 CrossRefGoogle Scholar
Hakala, P., Ramsay, G. 2003, A&A, submitted, astro-ph/0312343Google Scholar
Hameury, J.-M. & Lasota, J.-Р. 2002, A&A, 394, 231 Google Scholar
Hameury, J.-M., Lasota, J.-Р., & Dubus, G. 1999, MNRAS, 303, 39 Google Scholar
Hoard, D. W., Szkody, P., Froning, C. S., Long, K. S., & Knigge, C. 2003, AJ, 126, 2473 Google Scholar
Ishioka, R. et al. 2002, PASJ, 54, 581 Google Scholar
Kemp, J., Patterson, J., Thorstensen, J. R. et al. 2002, PASP, 114, 623 Google Scholar
King, A.R. 1997, MNRAS, 288, L16 Google Scholar
King, A.R., & Lasota, J.-Р. 1991, ApJ, 378, 674 Google Scholar
Koester, D. & Schoenberner, D. 1986, A&A, 154, 125 Google Scholar
Lasota, J.-Р. 2001, NewAR, 45, 449 Google Scholar
Lasota, J.-Р., Hameury, J.-M., & Huré, J.-M. 1995, ApJ, 302, L29 Google Scholar
Lasota, J.-Р., Kuulkers, E., & Charles, P. 1999, MNRAS, 305, 473 Google Scholar
Leach, R., Hessman, F.V., King, A.R., Stehle, R., & Mattei, J. 1999, MNRAS, 305, 225 Google Scholar
Mauche, C. W. & Mukai, K. 2002, ApJL, 566, L33 Google Scholar
Meyer, F. & Meyer-Hofmeister, E. 1994, A&A, 288, 175 Google Scholar
Patterson, J. 1980, ApJ, 241, 235 Google Scholar
Ramsay, G. et al. 2001a, A&A, 365, L288 Google Scholar
Ramsay, G. et al. 2001b, A&A, 365, L294 Google Scholar
Schreiber, M. R., Hameury, J.-M., & Lasota, J.-P. 2003, A&A, 410, 239 Google Scholar
Sion, E. M. & Urban, J. 2002, ApJ, 572, 456 Google Scholar
Thorstensen, J. R., Patterson, J., Kemp, J., & Vennes, S. 2002, PASP, 114, 1108 Google Scholar
Tovmassian, G.H., et al. 1998, A&A, 335, 227 Google Scholar
van Zyl, L. et al., 2004, MNRAS, in press, astro-ph/0401459Google Scholar
Welsh, W. F., Sion, E. M., Godon, P. 2003, ApJ, 599, 509 Google Scholar
Wheatley, P. J. & West, R. G. 2003, MNRAS, 345, 1009 Google Scholar
Wynn, G. A., King, A. R., & Horne, K. 1997, MNRAS, 286, 436 Google Scholar