| Original Articles |
|
|
|
|
Dynamical Evolution of Globular Clusters in the Galaxy |
| WU Zhen-Yu1,2;SHU Cheng-Gang1,3;CHEN Wen-Ping3 |
| 1Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030
2National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012
3Graduate Institute of Astronomy, National Central University, Taibei 32054 |
|
| Cite this article: |
|
WU Zhen-Yu, SHU Cheng-Gang, CHEN Wen-Ping 2003 Chin. Phys. Lett. 20 1648-1651 |
|
|
|
Abstract Given the initial conditions of spatial density distribution, velocity distribution and mass function, the dynamical evolution of globular clusters in the Milky Way is investigated in details by means of Monte Carlo simulations. Four dynamic mechanisms are considered: stellar evaporation, stellar evolution, tidal shocks due to both the disk and bulge, and dynamical friction. It is found that stellar evaporation dominates the evolution of low-mass clusters and all four are important for massive ones. For both the power-law and lognormal initial clusters mass functions, we can find the best-fit models which can match the present-day observations with their main features of the mass function almost unchanged after evolution of several Gyr. This implies that it is not possible to determine the initial mass function only based on the observed mass function today. The dispersion of the modeled mass functions mainly depends on the potential wells of host galaxies with the almost constant peaks, which is consistent with current observations.
|
| Keywords:
98.20.Gm
98.20.-d
|
|
|
Published: 01 September 2003
|
|
| PACS: |
98.20.Gm
|
(Globular clusters in the Milky Way)
|
| |
98.20.-d
|
(Stellar clusters and associations)
|
|
|
|
|
|
|
Viewed |
|
|
|
Full text
|
|
|
|
|
Abstract
|
|
|
|
|
