Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-29T12:49:46.906Z Has data issue: false hasContentIssue false
  • English
  • Français

FUSE Results on Magnetic CVs: VV Pup, YY Dra, LS Peg and DW UMa

Published online by Cambridge University Press:  12 April 2016

Paula Szkody ,
Donald W. Hoard ,
Albert P. Linnell ,
Knox Long ,
Gary Schmidt  and
Edward M. Sion
Paula Szkody
Affiliation:
Dept. of Astronomy, University of Washington, Box 351580, Seattle, WA 98195
Donald W. Hoard
Affiliation:
Dept. of Astronomy, University of Washington, Box 351580, Seattle, WA 98195
Albert P. Linnell
Affiliation:
Dept. of Astronomy, University of Washington, Box 351580, Seattle, WA 98195
Knox Long
Affiliation:
Space Telescope Science Insititute, 3700 San Martin Drive, Baltimore, MD 21218
Gary Schmidt
Affiliation:
Steward Observatory, University of Arizona, Tucson, AZ 85721
Edward M. Sion
Affiliation:
Department of Astronomy, Villanova University, Villanova, PA 19085

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.

In Cycles 2 and 3, we obtained FUSE observations of the Polar VV Pup, and the IP/SW Sex stars YY Dra, LS Peg and DW UMa. The spectra show a wide range of line intensities and structure. The phase-resolved spectra in each case reveal interesting properties about the hot accretion zones.

Type
Part 3. A. Accretion Plasma diagnostics - Observations
Information
International Astronomical Union Colloquium , Volume 190: Magnetic Cataclysmic Variables , 2004 , pp. 184 - 185
Copyright
Copyright © Astronomical Society of the Pacific 2004

References

Hoard, D. W., Szkody, P., Ishioka, R., Ferrano, L., Gänsicke, B. T., Schmidt, G. D., Kato, T., & Uemura, M. 2002, AJ, 124, 2238 Google Scholar
Rodriguez-Gil, P., Casares, J., Martinez-Pais, I. G., Hakala, P., & Steeghs, D. 2001, ApJ, 548, 49L CrossRefGoogle Scholar