The non-radially pulsating primary of the cataclysmic variable gw librae

Monthly Notices of the Royal Astronomical Society

Volumn 350, Issue 1, 2004, Pages 307-316

  Van Zyl, L ^a,b   Warner, B ^b   O'Donoghue, D ^c   Hellier, C ^a   Woudt, P ^b   Sullivan, D ^d   Pritchard, J ^e   Kemp, J ^f   Patterson, J ^f   Welsh, W ^g,h   Casares, J ⁱ   Shahbaz, T ^i,j   Van Der Hooft, F ^k   Vennes, S ^l  

^a KEELE UNIVERSITY   (United Kingdom)

^b UNIVERSITY OF CAPE TOWN   (South Africa)

^c SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^d VICTORIA UNIVERSITY OF WELLINGTON   (New Zealand)

^e UNIVERSITY OF CANTERBURY   (New Zealand)

^f Och Spine at New York Presbyterian Hospitals   (United States)

^g The University of Texas at Austin   (United States)

^h SAN DIEGO STATE UNIVERSITY   (United States)

ⁱ INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^j UNIVERSITY OF OXFORD   (United Kingdom)

^k UNIVERSITY OF AMSTERDAM   (Netherlands)

^l AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

more..

Author keywords

Novae, cataclysmic variables; Stars: individual: GW Librae; Stars: oscillations; White dwarfs

Indexed keywords

ACCRETION DISCS; ASTEROSEISMOLOGY; CATACLYSMIC VARIABLES; DWARF NOVAE; MULTIMODES; NOVAE CATACLYSMIC VARIABLES; PULSATING PRIMARY; STAR OSCILLATIONS; STAR: INDIVIDUAL: GW LIBRA; STARS: INDIVIDUAL: PROXIMA CENTAURI;

WHITE DWARFS;

EID: 2442514137     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07646.x     Document Type: Article

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