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X-ray Emission from Supermassive Black Holes in Elliptical Galaxies and Low Radiative-efficiency Accretion
Published online by Cambridge University Press: 25 May 2016
Abstract
We discuss the detection of hard, power-law emission components in the X-ray spectra of six nearby, giant elliptical galaxies observed with the ASCA satellite and its implication for low-radiative efficiency accretion models around the central, supermassive black holes.
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- Part II: Posters
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- Copyright © Astronomical Society of the Pacific 2000