High Energy Processes in Accreting Black Holes: Proceedings of a Workshop Held at Gräftåvallen, Sweden, 29 June-4 July, 1998Juri Poutanen, Roland Svensson |
Contents
Preface | xvii |
Xrays and Soft Gammarays from Seyferts Radio Galaxies | 16 |
Xray Energy Spectra of Galactic Black Hole Candidates | 39 |
Copyright | |
27 other sections not shown
Common terms and phrases
absorption accretion disk appear ASCA assumed average band BHCs black hole central cold Compton consistent continuum cooling corona Cyg X-1 density dependence detailed discussed dissipation distribution edge effects electrons emission energy et al excess expected Fabian factor Figure flare flow flux fraction frequency function Galactic galaxies geometry hard hard X-ray heating important increases indicate inner ionized iron ISBN lags light curves limit luminosity magnetic field mass MNRAS Nature Note objects observed optically panel parameters particle photon physical plasma possible Poutanen power law present processes produce properties QPOs radiation radio radius range reflection region relativistic scale scattering Seyfert shots shown significant similar soft soft photons spectral spectrum strong studies suggest Svensson temperature thermal thin typical University variability X-ray Zdziarski