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The non-radially pulsating primary of the cataclysmic variable GW Librae
Authors:L. van Zyl  B. Warner  D. O'Donoghue  C. Hellier  P. Woudt  D. Sullivan  J. Pritchard  J. Kemp  J. Patterson  W. Welsh  J. Casares  T. Shahbaz  F. van der Hooft   S. Vennes
Affiliation:Astrophysics Group, School of Chemistry and Physics, Keele University, Staffordshire ST5 5BG;Department of Astronomy, University of Cape Town, Rondebosch 7700, South Africa;South African Astronomical Observatory, PO Box 9, Observatory 7935, South Africa;School of Chemical and Physical Sciences, Victoria University, Box 600, Wellington, New Zealand;Department of Physics and Astronomy, University of Canterbury, Christchurch, New Zealand;Department of Astronomy, Columbia University, 550 West 120th Street, New York, NY 10027, USA;Department of Astronomy and McDonald Observatory, University of Texas at Austin, Austin, TX 78712, USA;Department of Astronomy, San Diego State University, 5500 Campanile Drive, San Diego, CA 92182-1221, USA;Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain;Department of Astrophysics, Oxford University, Keble Road, Oxford OX1 3RH;Astronomical Institute 'Anton Pannekoek', University of Amsterdam, and Center for High Energy Astrophysics, Kruislaan 403, NL-1098 SJ Amsterdam, the Netherlands;Department of Mathematics and Astrophysical Theory Centre, Australian National University, Canberra, ACT 0200, Australia
Abstract:
Keywords:stars: individual: GW Librae    novae, cataclysmic variables    stars: oscillations    white dwarfs
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