Supermassive Black Holes in Elliptical Galaxies: Switching from Very Bright to Very Dim

Abstract

Relativistic outflows (mainly observed in the radio) are a characteristic feature of both Galactic stellar mass black holes and supermassive black holes (SMBHs). Simultaneous radio and X-ray observations of Galactic sources have shown that the outflow is strong at low accretion rates, but it weakens dramatically or disappears completely at high accretion… (More)

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Cite this paper

@inproceedings{Churazov2005SupermassiveBH, title={Supermassive Black Holes in Elliptical Galaxies: Switching from Very Bright to Very Dim}, author={Eugene Churazov and Sergey Yu. Sazonov and Rachid Sunyaev and Williams Forman and C. Jones and H. J. B{\"o}hringer}, year={2005} }