A simple dynamical evolutionary model for ω Cen

被引：16

作者：

Giersz, M

Heggie, DC

机构：

[1] Polish Acad Sci, Nicolas Copernicus Astron Ctr, PL-00716 Warsaw, Poland

[2] Univ Edinburgh, Sch Math, Edinburgh EH9 3JZ, Midlothian, Scotland

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2003年 / 339卷 / 02期

关键词：

stellar dynamics; methods : miscellaneous; stars : luminosity function; mass function; globular clusters : individual : omega Cen;

D O I：

10.1046/j.1365-8711.2003.06191.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We construct a simple dynamical model of the massive globular cluster omega Cen. The model includes simple treatments of dynamical evolution in a galactic tide, and evolution of single stars. Binary stars and rotation are neglected. The model approximately fits observational data on the surface brightness profile, the profile of radial velocity dispersion, and the main sequence mass function at two radii.

引用

页码：486 / 490

页数：5

共 49 条

[21] The luminosity function of the globular cluster NGC 6397 near the limit of hydrogen burning [J].