XMM spectroscopy of the transient supersoft source RX J0513.9 - 6951: Probing the dynamic white dwarf photosphere

Monthly Notices of the Royal Astronomical Society

Volumn 364, Issue 2, 2005, Pages 462-474

  McGowan, K E ^a,b   Charles, P A ^c,d   Blustin, A J ^a   Livio, M ^e   O'Donoghue, D ^c   Heathcote, B ^f  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b LOS ALAMOS NATIONAL LABORATORY   (United States)

^c SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^d UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^e STScI   (United States)

^f Barfold Observatory   (Australia)

Author keywords

Binaries: close; Magellanic Clouds X rays: stars; Stars: individual: RX J0513.9 6951

Indexed keywords

LUMINANCE; MASS TRANSFER; SUPERNOVAE;

'CURRENT; BINARIES: CLOSE; MAGELLANIC CLOUD X-RAY: STAR; MAGELLANIC CLOUDS-X-RAYS; OPTICAL-; STAR: INDIVIDUAL: RX J0513.9-6951; STARS: INDIVIDUAL: PROXIMA CENTAURI; SURFACE HYDROGEN; X-RAY SOURCES; X-RAY:STARS; MAGELLANIC CLOUDS; STAR: INDIVIDUAL: RXJ0513.9 - 6951; THERMALLY UNSTABLE;

WHITE DWARFS;

EID: 28744456723     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09566.x     Document Type: Article

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