Study of Fe Kα lines in nonmagnetic cataclysmic variables using Chandra HEG data

Astrophysical Journal

Volumn 642, Issue 2 I, 2006, Pages 1042-1050

  Rana, V R ^a,d   Singh, K P ^a   Schlegel, E M ^b,e   Barrett, P E ^c,f  

^a TATA INSTITUTE OF FUNDAMENTAL RESEARCH   (India)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c STScI   (United States)

^d INDIAN INSTITUTE OF SCIENCE   (India)

^e UNIVERSITY OF TEXAS AT SAN ANTONIO   (United States)

^f JOHNS HOPKINS UNIVERSITY   (United States)

Author keywords

Accretion, accretion disks; Binaries: close; Novae, cataclysmic variables stars: individual (SS Cygni, SU Ursae Majoris, U Gemini, V426 Ophiuci, V603 Aquilae, WX Hydri); X rays: stars

Indexed keywords

EID: 33746071572     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/500316     Document Type: Article

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