MOCCA code for star cluster simulation: comparison with optical observations using COCOA

被引：0
|
作者：
Askar, Abbas [1 ]
Giersz, Mirek [1 ]
Pych, Wojciech [1 ]
Olech, Arkadiusz [1 ]
Hypki, Arkadiusz [1 ,2 ]
机构：
[1] Polish Acad Sci, Nicolaus Copernicus Astron Ctr, Ul Bartycka 18, PL-00716 Warsaw, Poland
[2] Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands
来源：
STAR CLUSTERS AND BLACK HOLES IN GALAXIES ACROSS COSMIC TIME | 2016年 / 10卷 / 312期
关键词：
stellar dynamics; globular clusters: general; methods: numerical;
D O I：
10.1017/S1743921315007991
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We introduce and present preliminary results from COCOA (Cluster simulatiOn Comparison with ObservAtions) code for a star cluster after 12 Gyr of evolution simulated using the MOCCA code. The COCOA code is being developed to quickly compare results of numerical simulations of star clusters with observational data. We use COCOA to obtain parameters of the projected cluster model. For comparison, a FITS file of the projected cluster was provided to observers so that they could use their observational methods and techniques to obtain cluster parameters. The results show that the similarity of cluster parameters obtained through numerical simulations and observations depends significantly on the quality of observational data and photometric accuracy.
引用
收藏
页码：262 / 263
页数：2
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