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Chandra HETG spectra of SS Cyg and U Gem in quiescence and outburst
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Mauche, C. W., Wheatley, P. J., Long, K. S., Raymond, J. C. and Szkody, P. (2005) Chandra HETG spectra of SS Cyg and U Gem in quiescence and outburst. In: The astrophysics of cataclysmic variables and related objects, Strasbourg, France, 11-16 Jul 2004. Published in: Astrophysics of Cataclysmic Variables and Related Objects, Volume 330 pp. 355-356. ISSN 9781583811931.
An open access version can be found in:Abstract
Chandra HETG spectra of the prototypical dwarf novae SS Cyg
and U Gem in quiescence and outburst are presented and discussed. When SS Cyg goes into outburst, it becomes dimmer in hard X-rays and displays a dramatic shift in its relative line strengths, whereas when U Gem goes into outburst, it becomes brighter in hard X-rays and displays only a minor shift in its relative line strengths. In both systems, the emission lines become significantly broader in outburst, signaling the presence of high velocity gas either in Keplerian orbits around the white dwarf or flowing outward from the system.
Item Type: | Conference Item (Paper) |
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Subjects: | Q Science > QB Astronomy |
Divisions: | Faculty of Science, Engineering and Medicine > Science > Physics |
Journal or Publication Title: | Astrophysics of Cataclysmic Variables and Related Objects |
Publisher: | Astronomical Society of the Pacific |
ISSN: | 9781583811931 |
Official Date: | 2005 |
Volume: | Volume 330 |
Page Range: | pp. 355-356 |
Status: | Not Peer Reviewed |
Publication Status: | Published |
Conference Paper Type: | Paper |
Title of Event: | The astrophysics of cataclysmic variables and related objects |
Type of Event: | Conference |
Location of Event: | Strasbourg, France |
Date(s) of Event: | 11-16 Jul 2004 |
Open Access Version: |
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