Galactic Nuclei

Details Galactic Nuclei Galactic Nuclei

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.235..319k&link_type=abstract

Astrophysics and Space Science, Volume 235, Issue 2, pp.319-327

Astronomy and Astrophysics

Astrophysics

7

Scientific paper

Application of standard accretion-disk theory to the central parts of galactic disks implies that galactic nuclei should pass quasi-periodically through stages of (i) gravitational instability (Starburst), (ii) non-thermal disk activity (LINER), and (iii) central-plane nuclear burning (AGN). Nuclear disks can have large mass-to-light ratios, and store large masses at high (Keplerian) rotation velocities. Aburning disk can explain all the phenomena commonly attributed to a supermassive Black Hole.

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