Properties of the hard X-ray radiation from Cygnus X-1 and 1E1740.7 - 2942

Monthly Notices of the Royal Astronomical Society

Volumn 292, Issue 3, 1997, Pages 651-656

  Kuznetsov, S ^a,b,c   Gilfanov, M ^a,c   Churazov, E ^a,c   Sunyaev, R ^a,c   Korel, I ^a,b   Khavenson, N ^a   Dyachkov, A ^a   Chulkov, I ^a   Ballet, J ^d   Laurent, P ^d   Vargas, M ^d   Goldwurm, A ^d   Roques, J P ^e   Jourdain, E ^e   Bouchet, L ^e   Borrel, V ^e  

^a Russian Academy of Sciences ^*  (Russian Federation)

^b MOSCOW INSTITUTE OF PHYSICS AND TECHNOLOGY   (Russian Federation)

^c MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^d UNIVERSITÉ PARIS DIDEROT   (France)

^e IRAP   (France)

Author keywords

Accretion, accretion discs; Binaries: close; Gamma rays: observations; Stars: individual: 1E1740.72942; Stars: individual: Cyg X 1; X rays: stars

Indexed keywords

GAMMA RAYS; LUMINANCE; STARS;

ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; GAMMA-RAYS:OBSERVATIONS; HARD X RAY; PROPERTY; STAR: INDIVIDUAL: 1E1740.72942; STARS: INDIVIDUAL: CYG X-1; STARS: INDIVIDUAL: PROXIMA CENTAURI; X-RAY LUMINOSITY; X-RAY:STARS;

HARDNESS;

EID: 0009128989     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/292.3.651     Document Type: Article

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