The broad iron Kα line of Cygnus X-1 as seen by XMM-Newton in the EPIC-pn modified timing mode

Astronomy and Astrophysics

Volumn 533, Issue , 2011, Pages

  Duro, R ^a   Dauser, T ^a   Wilms, J ^a   Pottschmidt, K ^b,c   Nowak, M A ^d   Fritz, S ^a,e   Kendziorra, E ^e   Kirsch, M G F ^f   Reynolds, C S ^g   Staubert, R ^e  

^a UNIVERSITY OF ERLANGEN NUREMBERG   (Germany)

^b NASA GODDARD SPACE FLIGHT CENTER   (United States)

^c NATIONAL SPACE SCIENCE AND TECHNOLOGY CENTER   (United States)

^d MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^e UNIVERSITY OF TÜBINGEN   (Germany)

^f ESA ESOC   (Germany)

^g UNIVERSITY OF MARYLAND   (United States)

Author keywords

Black hole physics; Gravitation; X rays: binaries

Indexed keywords

ACCRETION DISKS; BLACK HOLE PHYSICS; BLACK HOLES; COMPTON BROADENING; DROP-OUT; LOWER ENERGIES; POWER-LAW; SIGNAL TO NOISE; X-RAYS: BINARIES; XMM-NEWTON;

SIGNAL TO NOISE RATIO; STARS;

GRAVITATION;

EID: 80052519733     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117446     Document Type: Article

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