The Proposed Black Holes around us

Physics

Scientific paper

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Black Holes, Supermassive Black Holes, Black-Hole Candidates

Scientific paper

This chapter combines two of my contributions to MG 11: an analysis of the proposed supermassive black holes at the centers of galaxies which are thought to give rise to the quasar phenomenon, and an analysis of the stellar-mass black-hole candidates (BHCs) - typically a million times smaller in mass - which behave similarly to neutron stars, and are often called 'microquasars'. For both source types, I shall argue that the black-hole interpretation meets with serious inconsistencies, and that instead, we deal with non-collapsed, rotating, strongly magnetized concentrations of matter, similar to ordinary stars and neutron stars.

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