Central Black Holes and Dark Halos in Elliptical Galaxies
1995 ◽
Vol 164
◽
pp. 215-225
Keyword(s):
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.
1997 ◽
Vol 163
◽
pp. 620-625
◽
Keyword(s):
1992 ◽
Vol 259
(1)
◽
pp. 27P-30P
◽
2009 ◽
Vol 5
(H15)
◽
pp. 269-270
2015 ◽
Vol 815
(1)
◽
pp. 21
◽
Keyword(s):
2000 ◽
Vol 84
(23)
◽
pp. 5258-5260
◽
2003 ◽
Vol 209
◽
pp. 635-636
2005 ◽
Vol 363
(1828)
◽
pp. 705-713
Keyword(s):
2011 ◽
Vol 20
(10)
◽
pp. 1937-1940
Keyword(s):