Resolving the composite Fe Kα emission line in the galactic black hole Cygnus X-1 with Chandra

Astrophysical Journal

Volumn 578, Issue 1 I, 2002, Pages 348-356

  Miller, J M ^a   Fabian, A C ^b   Wijnands, R ^a   Remillard, R A ^a   Wojdowski, P ^a   Schulz, N S ^a   Di Matteo, T ^c   Marshall, H L ^a   Canizares, C R ^a   Pooley, D ^a   Lewin, W H G ^a  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Accretion, accretion disks; Black hole physics; Relativity; Stars: individual (Cygnus X 1); X rays: binaries; X rays: individual (Cygnus X 1)

Indexed keywords

EID: 0005325920     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/342466     Document Type: Article

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