The defining characteristics of intermediate polars - The case of three-candidate systems

Monthly Notices of the Royal Astronomical Society

Volumn 387, Issue 3, 2008, Pages 1157-1162

  Ramsay, Gavin ^a   Wheatley, Peter J ^b   Norton, A J ^c   Hakala, Pasi ^d   Baskill, Darren ^e,f  

^a ARMAGH OBSERVATORY   (United Kingdom)

^b UNIVERSITY OF WARWICK   (United Kingdom)

^c OPEN UNIVERSITY   (United Kingdom)

^d UNIVERSITY OF TURKU   (Finland)

^e UNIVERSITY OF LEICESTER   (United Kingdom)

^f ROYAL GREENWICH OBSERVATORY   (United Kingdom)

Author keywords

Binaries: close; Novae, cataclysmic variables; Stars: individual: EI UMa; Stars: individual: LS Peg; Stars: individual: V426 Oph; X rays: binaries

Indexed keywords

WHITE DWARFS; X RAY ANALYSIS; X RAY SPECTROGRAPHS;

BINARIES: CLOSE; INTERMEDIATE POLARS; NOVAE CATACLYSMIC VARIABLES; STAR: INDIVIDUAL: EI UMA; STAR: INDIVIDUAL: LS PEG; STAR: INDIVIDUAL: V426 OPH; STARS: INDIVIDUAL: PROXIMA CENTAURI; X-RAYS: BINARIES;

MODULATION;

EID: 45249115903     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13299.x     Document Type: Article

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