Papadaki, C., Boffin, H. (Henri), 1965- and Steeghs, D. (Danny), 1972- (2005) Simultaneous Doppler maps of IP Peg in outburst. In: The astrophysics of cataclysmic variables and related objects, Strasbourg, France, 11-16 Jul 2004. Published in: Astronomical Society of the Pacific Conference Series, Vol.330 p. 373.

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Abstract

IP Pegasi is an eclipsing dwarf nova lying above the period gap with an orbital period of 3.8h. It is the first cataclysmic variable to show evidence of spiral arms in its accretion disc. We present new time-resolved echelle spectroscopic observations of IP Peg, covering the 3900-7700 Angstrom range. This allows us to produce simultaneous Doppler Maps in 9 emission lines.

Item Type:	Conference Item (Paper)
Subjects:	Q Science > QB Astronomy
Divisions:	Faculty of Science > Physics
Library of Congress Subject Headings (LCSH):	Cataclysmic variable stars, Eclipsing binaries, Dwarf novae
Journal or Publication Title:	Astronomical Society of the Pacific Conference Series
Publisher:	Astronomical Society of the Pacific
ISSN:	1050-3390
Date:	2005
Volume:	Vol.330
Page Range:	p. 373
Status:	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
References:	Piche, F. & Szkody, P. 1989, AJ, 98, 2225 Spruit, H.C. 1998, astro-ph/9806141 Steeghs, D., Harlaftis, E. T. & Horne, K. 1997, MNRAS, 290, L28 Wolf, S. et al. 1993, A&A, 273, 160
URI:	http://wrap.warwick.ac.uk/id/eprint/50097

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