Modelling the broad-band spectral energy distribution of the microquasars XTE J1550-564 and H 1743-322

Monthly Notices of the Royal Astronomical Society

Volumn 384, Issue 1, 2008, Pages 440-448

  Xue, Yongquan ^a   Wu, Xue Bing ^b   Cui, Wei ^a,b  

^a PURDUE UNIVERSITY   (United States)

^b PEKING UNIVERSITY   (China)

Author keywords

Accretion, accretion discs; Black hole physics; X rays: binaries; X rays: individual: H 1743 322; X rays: individual: XTE J1550 564

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; GRAVITATION; SPECTROSCOPY; SYNCHROTRONS; X RAY SCATTERING;

ACCRETION: ACCRETION DISKS; BLACK HOLE PHYSICS; JET EMISSIONS; SPECTRAL ENERGY DISTRIBUTION; SYNCHROTRON EMISSION; X-RAY: INDIVIDUAL: H 1743-322; X-RAY: INDIVIDUAL: XTE J1550-564; X-RAYS: BINARIES; X-RAYS: INDIVIDUAL;

SYNCHROTRON RADIATION;

EID: 38749102740     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12721.x     Document Type: Article

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