On the hypothesis of ejection of supermassive black holes from centers of galaxies and its application to quasar-galaxy associations

Details On the hypothesis of ejection of supermassive black holes from centers of galaxies and its application to quasar-galaxy associations On the hypothesis of ejection of supermassive black holes from centers of galaxies and its application to quasar-galaxy associations

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..93...79k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 93, no. 1, June 1983, p. 79-85.

Astronomy and Astrophysics

Astronomy

3

Accretion Disks, Black Holes (Astronomy), Galactic Nuclei, Quasars, Astronomical Models, Red Shift

Scientific paper

It is argued that accreting supermassive black holes ejected from centers of galaxies are the likely models for the quasars observed in association with galaxies. Also pointed out are the implications of a recent suggestion by Horák (1982) to account for the excess redshifts of such quasars due to a combined effect of peculiar Doppler-motion and the gravitational field

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