Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-29T12:44:41.521Z Has data issue: false hasContentIssue false
  • English
  • Français

Discovery of 15-second Oscillations in HST observations of W Sge following the 2001 Outburst

Published online by Cambridge University Press:  12 April 2016

S. Araujo-Betancor ,
C. Knigge ,
T. R. Marsh ,
R. I. Hynes ,
D. Steeghs  and
K. S. Long
S. Araujo-Betancor
Affiliation:
University of Southampton, Dept. of Physics & Astronomy, Southampton SO17 1BJ, UK
C. Knigge
Affiliation:
University of Southampton, Dept. of Physics & Astronomy, Southampton SO17 1BJ, UK
T. R. Marsh
Affiliation:
University of Southampton, Dept. of Physics & Astronomy, Southampton SO17 1BJ, UK
R. I. Hynes
Affiliation:
University of Southampton, Dept. of Physics & Astronomy, Southampton SO17 1BJ, UK
D. Steeghs
Affiliation:
University of Southampton, Dept. of Physics & Astronomy, Southampton SO17 1BJ, UK
K. S. Long
Affiliation:
Space Telescope Science Institute, Baltimore, MD 21218, USA

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 report the discovery of 15 s oscillations in HST/STIS far-UV spectroscopic observations of WZ Sge in decline, one month after the start of its 2001 outburst. We discuss the implications of this finding for both the magnetic and pulsating white dwarf models that have been proposed to account for the 28 s oscillations.

Type
Part 3. A. Accretion Plasma diagnostics - Observations
Information
International Astronomical Union Colloquium , Volume 190: Magnetic Cataclysmic Variables , 2004 , pp. 170 - 171
Copyright
Copyright © Astronomical Society of the Pacific 2004

References

Patterson, J., Richman, H., Kemp, J., & Mukai, K. 1998, PASP, 110, 403 Google Scholar
Skidmore, W., Welsh, W. F., Wood, J. H., Catalán, M. S., & Horne, K. 1999, MNRAS, 310, 750 Google Scholar
Warner, B., & Woudt, P. A. 2002, MNRAS, in press (astro-ph/0204484)Google Scholar