Hostname: page-component-848d4c4894-wzw2p Total loading time: 0 Render date: 2024-05-14T20:55:48.353Z Has data issue: false hasContentIssue false
  • English
  • Français

Breaking the 100 MG Barrier: The First High Field Magnetic CV

Published online by Cambridge University Press:  12 April 2016

Paula Szkody ,
Gary D. Schmidt ,
Paul S. Smith ,
Andrew Silber ,
D.W. Hoard ,
Gaghik Tovmassian ,
B.T. Gänsicke  and
D. de Martino
Paula Szkody
Affiliation:
Dept. of Astronomy, University of Washington, Box 351580, Seattle, WA 98195
Gary D. Schmidt
Affiliation:
Steward Observatory, University of Arizona, Tucson, AZ 85721
Paul S. Smith
Affiliation:
Steward Observatory, University of Arizona, Tucson, AZ 85721
Andrew Silber
Affiliation:
Dept. of Astronomy, University of Washington, Box 351580, Seattle, WA 98195
D.W. Hoard
Affiliation:
Dept. of Astronomy, University of Washington, Box 351580, Seattle, WA 98195
Gaghik Tovmassian
Affiliation:
Instituto de Astronomia, UNAM, Apdo. Post 877, 22860, Ensenada, B.C., Mexico
B.T. Gänsicke
Affiliation:
Universitat-Sternwarte, Geismarlandstrasse 11, D-37083, Gottingen, Germany
D. de Martino
Affiliation:
IUE Observatory, VILSPA-ESA, P.O. Box 50727, E-28080 Madrid, Spain

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.

We present results from IUE and optical spectra, optical photometry and circular polarimetry during high and low states of the highly luminous soft X-ray cataclysmic variable AR UMa that identifies the primary in this system as a white dwarf with a magnetic field of 230 MG. The high magnetic field likely threads accretion blobs all the way from the secondary to below the surface of the white dwarf, resulting in a lack of polarised cyclotron emission and an extreme soft-X-ray luminosity during the high state.

Type
Part 9. Accretion Curtains and Funnels
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 409 - 412
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Cropper, M. 1990, Sp. Sci. Rev., 54, 195 CrossRefGoogle Scholar
Liebert, J., Bergeron, P., Schmidt, G.D., & Saffer, R.A. 1993, ApJ, 418, 426 CrossRefGoogle Scholar
Remillard, R.A., Schachter, J.F., Silber, A.D. & Slane, P. 1994, ApJ, 426, 288 CrossRefGoogle Scholar
Schmidt, G.D., Stockman, H.S., & Grandi, S.A. 1986, ApJ, 300, 804 CrossRefGoogle Scholar
Schmidt, G.D., Allen, R., Smith, P., & Liebert, J. 1996a, ApJ, in pressGoogle Scholar
Schmidt, G.D., Szkody, P., Smith, P., Silber, A., Tovmassian, G., Hoard, D.W., Gänsicke, B.T. & de Martino, D. 1996b, ApJ, in pressGoogle Scholar