Corona, jet, and relativistic line models for Suzaku/RXTE/Chandra-HETG observations of the cygnus X-1 hard state

Astrophysical Journal

Volumn 728, Issue 1, 2011, Pages

  Nowak, Michael A ^a   Hanke, Manfred ^b   Trowbridge, Sarah N ^a   Markoff, Sera B ^c   Wilms, Jörn ^b   Pottschmidt, Katja ^d   Coppi, Paolo ^e   Maitra, Dipankar ^c,f   Davis, John E ^a   Tramper, Frank ^c  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^b UNIVERSITY OF ERLANGEN NUREMBERG   (Germany)

^c UNIVERSITY OF AMSTERDAM   (Netherlands)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

^e YALE UNIVERSITY   (United States)

^f UNIVERSITY OF MICHIGAN   (United States)

Author keywords

Accretion, accretion disks; Black hole physics; Radiation mechanisms: non thermal; X rays: binaries

Indexed keywords

EID: 84891207361     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/728/1/13     Document Type: Article

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