An XMM-Newton observation of the nova-like variable UX UMa: Spatially and spectrally resolved two-component X-ray emission

Monthly Notices of the Royal Astronomical Society

Volumn 348, Issue 3, 2004, Pages

  Pratt, G W ^a,b   Mukai, K ^c,g   Hassall, B J M ^d   Naylor, T ^e   Wood, J H ^f  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c NASA GODDARD SPACE FLIGHT CENTER   (United States)

^d UNIVERSITY OF CENTRAL LANCASHIRE   (United Kingdom)

^e UNIVERSITY OF EXETER   (United Kingdom)

^f KEELE UNIVERSITY   (United Kingdom)

^g UNIVERSITIES SPACE RESEARCH ASSOCIATION   (United States)

Author keywords

Binaries: eclipsing; Novae, cataclysmic variables; Stars: individual: UX UMa; X rays: stars

Indexed keywords

BOUNDARY LAYERS; ELECTROMAGNETIC WAVE EMISSION; MASS TRANSFER; STARS;

BINARIES:ECLIPSING; NOVAE CATACLYSMIC VARIABLES; OPTICAL REGIONS; PLASMA MODELING; STAR: INDIVIDUAL: UX UMA; STARS: INDIVIDUAL: PROXIMA CENTAURI; TWO-COMPONENT; X-RAY EMISSION; X-RAY:STARS; XMM-NEWTON OBSERVATIONS;

X RAY SCATTERING;

EID: 1542357740     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07574.x     Document Type: Article

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