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Dynamical modeling of the Arches cluster using Fokker-Planck calculations

Published online by Cambridge University Press:  07 March 2016

Joowon Lee  and
Jihye Shin
Joowon Lee
Affiliation:
School of Space Research, Kyung Hee University, Yongin, Gyeonggi 446-701, Korea email: joowon.lee@khu.ac.kr
Jihye Shin
Affiliation:
Kavli Institute for Astronomy and Astrophysics, Peking University, 5 Yiheyuan Road, Haidian District, Beijing 100871, China
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Abstract

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The Arches cluster is a young, compact, and massive star cluster located in ~30pc away from the Galactic Center in projection. The cluster is located in the extreme environment of the Galactic Center, making it an excellent target for understanding the effects of star-forming environment on the mass function of star clusters. In this study, we estimate the initial condition (mass, concentration parameter, and galactocentric radius) of the Arches cluster by comparing Fokker-Planck calculations with observed velocity dispersion, surface density and mass function data.

Keywords

Galaxy: globular clusters: individual(Arches)Galaxy: kinematics and dynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S312: Star Clusters and Black Holes in Galaxies across Cosmic Time , August 2014 , pp. 241 - 242
Copyright
Copyright © International Astronomical Union 2016 

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