A relativistic Fe Kα emission line in the intermediate-luminosity BeppoSAX spectrum of the galactic microquasar V4641 SGR

Astrophysical Journal

Volumn 577, Issue 1 II, 2002, Pages

  Miller, J M ^a   Fabian, A C ^b   In 't Zand, J J M ^c,d   Reynolds, C S ^e   Wijnands, R ^a   Nowak, M A ^a   Lewin, W H G ^a  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c UTRECHT UNIVERSITY   (Netherlands)

^d SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^e Bldg 142   (United States)

Author keywords

Black hole physics; X rays: individual (V4641 Sagittarii); X rays: stars

Indexed keywords

EID: 0041970889     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/344047     Document Type: Article

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