INTEGRAL and RXTE monitoring of GRS 1758-258 in 2003 and 2004 A transition from the dim soft state to the hard state

Astronomy and Astrophysics

Volumn 452, Issue 1, 2006, Pages 285-294

  Pottschmidt, K ^a   Chernyakova, M ^b,e   Zdziarski, A A ^c   Lubinski P ^b,c   Smith, D M ^d   Bezayiff, N ^d  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF GENEVA   (Switzerland)

^c NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e LEBEDEV PHYSICAL INSTITUTE   (Russian Federation)

Author keywords

Black hole physics; Gamma rays: observations; Stars: individual: GRS 1758 258; X rays: binaries; X rays: general

Indexed keywords

ASTROPHYSICS; GAMMA RAY PRODUCTION; LUMINESCENCE; MATHEMATICAL MODELS; SPECTRUM ANALYSIS; X RAYS;

BLACK HOLE PHYSICS; GAMMA RAYS: OBSERVATIONS; STARS: INDIVIDUAL: GRS 1758-258; X-RAYS: BINARIES; X-RAYS: GENERAL;

GALAXIES;

EID: 33744963555     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054077     Document Type: Article

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