6. SUGGESTIONS FOR FURTHER READING
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The search for BHs is reviewed in the following papers:
Kormendy, J., & Richstone, D.
Ann. Rev. Astr. Astrophys.
33, 581 (1995)
Richstone, D., et al.
Nature
395, A14 (1998)
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In the following papers, quasar energetics are used to predict the masses of
dead AGN engines:
Soltan, A.
M.N.R.A.S.
200, 115 (1982)
Chokshi, A., & Turner, E. L.
M.N.R.A.S.
259, 421 (1992)
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Dynamical models of galaxies as linear combinations of individual orbits are
discussed in
Schwarzschild, M.
Astrophys. J.
232, 236 (1979)
Richstone, D. O., & Tremaine, S.
Astrophys. J.
327, 82 (1988)
van der Marel, R. P., Cretton, N., de Zeeuw, P. T., & Rix, H.-W.
Astrophys. J.
493, 613 (1998)
Gebhardt, K., et al.
Astron. J.
119, 1157 (2000)
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The BH detection in NGC 3115 is discussed in
Kormendy, J., & Richstone, D.
Astrophys. J.
393, 559 (1992)
Kormendy, J., et al.
Astrophys. J. Lett.
459, L57 (1996)
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The BH detection in M 31 is discussed in
Dressler, A., & Richstone, D. O.
Astrophys. J.
324, 701 (1988)
Kormendy, J.
Astrophys. J.
325, 128 (1988)
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Tremaine's model for the double nucleus of M 31 and new evidence for that
model are in
Tremaine, S.
Astron. J.
110, 628 (1995)
Kormendy, J., & Bender, R.
Astrophys. J.
522, 772 (1999)
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HST spectroscopy of the double nucleus of M 31 is presented in
Statler, T. S., King, I. R., Crane, P., & Jedrzejewski, R. I.
Astron. J.
117, 894 (1999)
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The following are thorough reviews of the Galactic center:
Genzel, R., Hollenbach, D., & Townes, C. H.
Rep. Prog. Phys.
57, 417 (1994)
Morris, M., & Serabyn, E.
Ann. Rev. Astr. Astrophys.
34, 645 (1996)
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The latest measurement of the size of the Galactic center radio source is by
Lo, K. Y., Shen, Z.-Q., Zhao, J.-H., & Ho, P. T. P.
Astrophys. J. Lett.
508, L61 (1998)
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The remarkable proper motion measurements of stars near Sgr A* and resulting
conclusions about the Galactic center BH are presented in
Genzel, R., Eckart, A., Ott, T., & Eisenhauer, F.
M.N.R.A.S.
291, 219 (1997)
Ghez, A. M., Klein, B. L., Morris, M., & Becklin, E. E.
Astrophys. J.
509, 678 (1998)
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Arguments against compact dark star clusters in NGC 4258 and the Galaxy are
presented in
Maoz, E.
Astrophys. J. Lett.
494, L181 (1998)