Hostname: page-component-77c89778f8-m8s7h Total loading time: 0 Render date: 2024-07-23T10:17:00.260Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Published online by Cambridge University Press:  07 March 2016

Abbas Askar ,
Mirek Giersz ,
Wojciech Pych ,
Arkadiusz Olech  and
Arkadiusz Hypki
Abbas Askar
Affiliation:
Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warsaw, Poland email: askar@camk.edu.pl
Mirek Giersz
Affiliation:
Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warsaw, Poland email: askar@camk.edu.pl
Wojciech Pych
Affiliation:
Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warsaw, Poland email: askar@camk.edu.pl
Arkadiusz Olech
Affiliation:
Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warsaw, Poland email: askar@camk.edu.pl
Arkadiusz Hypki
Affiliation:
Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warsaw, Poland email: askar@camk.edu.pl Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden, The Netherlands
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Keywords

stellar dynamicsglobular clusters: generalmethods: numerical
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. 262 - 263
Copyright
Copyright © International Astronomical Union 2016 

References

Giersz, M., Heggie, D. C., Hurley, J. R., & Hypki, A. 2013, MNRAS, 431, 2184CrossRefGoogle Scholar
Hypki, A. & Giersz, M. 2013, MNRAS, 429, 1221Google Scholar