Why do some intermediate polars show soft X-ray emission? A survey of XMM-Newton spectra

Astrophysical Journal

Volumn 663, Issue 2 I, 2007, Pages 1277-1284

  Evans, P A ^a,b   Hellier, Coel ^a  

^a KEELE UNIVERSITY   (United Kingdom)

^b UNIVERSITY OF LEICESTER   (United Kingdom)

Author keywords

Accretion, accretion disks; Novae, cataclysmic variables; X rays: binaries

Indexed keywords

EID: 34547431026     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/518552     Document Type: Article

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