Improved Evidence for a Black Hole in M32 fromHST/FOS Spectra. II. Axisymmetric Dynamical Models

1998 ◽  
Vol 493 (2) ◽  
pp. 613-631 ◽  
Author(s):  
Roeland P. van der Marel ◽  
N. Cretton ◽  
P. Tim de Zeeuw ◽  
Hans‐Walter Rix
Keyword(s):  
1985 ◽  
Vol 296 ◽  
pp. 370 ◽  
Author(s):  
D. O. Richstone ◽  
S. Tremaine

1977 ◽  
Vol 218 ◽  
pp. L109 ◽  
Author(s):  
G. Illingworth ◽  
I. R. King
Keyword(s):  

2004 ◽  
Vol 220 ◽  
pp. 179-180 ◽  
Author(s):  
Glenn van de Ven ◽  
Ellen Verolme ◽  
Michele Cappellari ◽  
Tim de Zeeuw

We have developed a method to construct realistic triaxial dynamical models for elliptical galaxies, allowing us to derive best-fitting parameters, such as the mass-to-light ratio and the black hole mass, and to study the orbital structure. We use triaxial theoretical Abel models to investigate the robustness of the method.


2010 ◽  
Vol 710 (2) ◽  
pp. 1063-1088 ◽  
Author(s):  
Roeland P. van der Marel ◽  
Jay Anderson

2015 ◽  
Vol 450 (1) ◽  
pp. 128-144 ◽  
Author(s):  
Daniel Alf Drehmer ◽  
Thaisa Storchi-Bergmann ◽  
Fabricio Ferrari ◽  
Michele Cappellari ◽  
Rogemar A. Riffel

2013 ◽  
Vol 770 (2) ◽  
pp. 86 ◽  
Author(s):  
Jonelle L. Walsh ◽  
Aaron J. Barth ◽  
Luis C. Ho ◽  
Marc Sarzi

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