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Central Black Holes and Dark Halos in Elliptical Galaxies

Published online by Cambridge University Press:  07 August 2017

P.T. De Zeeuw
P.T. De Zeeuw*
Affiliation:
Sterrewacht Leiden, Postbus 9513, 2300 RA Leiden, The Netherlands (tim@strw.LeidenUniv.nl)

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Studies of the mass–to–light ratio M/L as a function of radius in a galaxy usually focus on: a) the existence of dark matter in and around galaxies, and b) the presence of massive black holes in their nuclei. Here we concentrate on elliptical galaxies, and summarize some recent work in both areas. We refer to more extensive reviews for earlier developments (Schwarzschild, 1954; Trimble, 1987; Ashman, 1992; Kormendy, 1993). A third area of interest is the behavior of the stellar populations as a function of radius, and its effect on M/L (e.g., Peletier, 1989). We will not discuss this here.

Type
Session 5: Dark Matter in Galaxies
Information
Symposium - International Astronomical Union , Volume 164: Stellar Populations , 1995 , pp. 215 - 225
Copyright
Copyright © Kluwer 1995 

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