Accretion mode changes in QS Tel (RE 1938 - 461): EUVE, ROSAT and optical observations

Monthly Notices of the Royal Astronomical Society

Volumn 280, Issue 4, 1996, Pages 1121-1142

  Rosen, S R ^a   Mittaz, J P D ^b   Buckley, D A ^c   Layden, A C ^d   Clayton, K L ^a   McCain, C ^e   Wynn, G A ^a   Sirk, M M ^f   Osborne, J P ^a   Watson, M G ^a  

^a UNIVERSITY OF LEICESTER   (United Kingdom)

^b UNIVERSITY COLLEGE LONDON   (United Kingdom)

^c SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^d CERRO TOLOLO INTER AMERICAN OBSERVATORY   (Chile)

^e AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^f UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Accretion, accretion discs; Binaries: close; Novae, cataclysmic variables; Stars: individual: QS Tel (RE 1938 461); X rays: stars

Indexed keywords

OPTICAL CORRELATION; PHOTOMETRY; STARS;

ACCRETION FLOW; ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; LIGHT CURVES; MODE CHANGES; NOVAE CATACLYSMIC VARIABLES; SPECTRA'S; STAR: INDIVIDUAL: QS TEL (RE 1938-461); STARS: INDIVIDUAL: PROXIMA CENTAURI; X-RAY:STARS;

SURVEYS;

EID: 0001145725     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/280.4.1121     Document Type: Article

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