Analytical models for galactic nuclei

被引:526
作者
Zhao, HS
机构
[1] Max-Planck-Inst. f. Astrophysik, 85740 Garching bei München
关键词
methods; analytical; celestial mechanics; stellar dynamics; galaxies; kinematics and dynamics; nuclei;
D O I
10.1093/mnras/278.2.488
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
I present a general family of dynamical models with simple analytical potential-density pairs suited to modelling galactic bulges and nuclei with double power-law radial density profiles and an optional central black hole. Analytical expressions for the potential and velocity dispersion of these models are given for the spherical case. Many previously known analytical spherical models, including the recent gamma/eta-models by Dehnen and Tremaine et al., are special cases of this family. The family also forms a complete set for constructing general galaxy models or solving Poisson's equation in the non-spherical case. In particular, a generalized Clutton-Brock and Hernquist-Ostriker orthogonal basis set is given.
引用
收藏
页码:488 / 496
页数:9
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