Rotational broadening and Doppler tomography of the quiescent X-ray nova Centaurus X-4

Monthly Notices of the Royal Astronomical Society

Volumn 334, Issue 1, 2002, Pages 233-240

  Torres, M A P ^a,b,c   Casares, J ^b   Martinez Pais I G ^a,b   Charles, P A ^d,e  

^a UNIVERSIDAD DE LA LAGUNA   (Spain)

^b INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^c UNIVERSITY COLLEGE CORK   (Ireland)

^d UNIVERSITY OF OXFORD   (United Kingdom)

^e UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

Author keywords

Accretion, accretion discs; Binaries: close; Novae, cataclysmic variables; Stars: individual: Centaurus X 4; X rays: stars

Indexed keywords

EID: 0041591509     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2002.05521.x     Document Type: Article

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