The dynamical evidence for black holes (BHs) in galactic nuclei is reviewed, with emphasis on recent improvements in spatial resolution, methods for analyzing galaxy spectra and dynamical modeling. M31, M32 and M87 are discussed in some detail.
- Pub Date:
- October 1994
- To appear in Highlights of Astronomy, Vol. 10, Proc. of the XXIInd General Assembly of the IAU, The Hague, August 1994, ed.~J.~Bergeron, Kluwer Academic Publishers. Format : 4 pages, no figures, PostScript file