Possible power source of Seyfert galaxies and QSOs

Details Possible power source of Seyfert galaxies and QSOs Possible power source of Seyfert galaxies and QSOs

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.254..295h&link_type=abstract

Nature, vol. 254, Mar. 27, 1975, p. 295-298.

Astronomy and Astrophysics

Astronomy

279

Black Holes (Astronomy), Mass Transfer, Quasars, Seyfert Galaxies, Galactic Nuclei, Gas Flow, Roche Limit, Stellar Mass, Stellar Mass Ejection

Scientific paper

The possible presence of massive black holes in the nuclei of galaxies has been suggested many times. In addition, there is considerable observational evidence for high stellar densities in these nuclei. I show that the tidal breakup of stars passing within the Roche limit of a black hole initiates a chain of events that may explain many of the observed principal characteristics of QSOs and the nuclei of Seyfert galaxies.

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