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Formation and evolution of sub-galactic structures in a cosmological context

Published online by Cambridge University Press:  09 May 2016

Kyungwon Chun
Affiliation:
School of Space Research, Kyung Hee University, Yongin, Gyeonggi, 446-701, Korea email: kwchun@khu.ac.kr
Jihye Shin
Affiliation:
Kavli Institute for Astronomy and Astrophysics, Peking University, 5 Yiheyuan Road, Haidian District, Beijing 100871, China email: jhshin.jhshin@gmail.com
Sungsoo S. Kim
Affiliation:
School of Space Research, Kyung Hee University, Yongin, Gyeonggi, 446-701, Korea email: kwchun@khu.ac.kr Department of Astronomy and Space Science, Kyung Hee University, Yongin, Gyeonggi, 446-701, Korea email: sungsoo.kim@khu.ac.kr
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Abstract

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In this study, we aim to trace formation of the primordial globular cluster, ultra faint dwarf galaxy, and ultra compact dwarf in a cosmological context of a high-resolution hydrodynamic zoom-in simulation. We show that the baryon-dominated systems have experienced more interactions with the mini halos before infalling to the main halo.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2016 

References

Ferland, G. J., Korista, K. T., Verner, D. A., Ferguson, J. W., Kingdon, J. B., & Verner, E. M. 1998, PASP, 110, 761CrossRefGoogle Scholar
Haardt, F. & Madau, P. 1996, ApJ, 461, 20CrossRefGoogle Scholar
Hahn, O. & Abel, T. 2011, MNRAS, 415, 2101CrossRefGoogle Scholar
Knollmann, S. R. & Knebe, A. 2009, ApJs, 182, 608CrossRefGoogle Scholar
Saitoh, T. R., Daisaka, H., Kokubo, E., Makino, J., Okamoto, T., Tomisaka, K., Wada, K., & Yoshida, N. 2008, PASJ, 60, 667CrossRefGoogle Scholar
Sawala, T., Scannapieco, C., Maio, U., & White, S. 2010, MNRAS, 402, 1599CrossRefGoogle Scholar
Springel, V. 2005, MNRAS, 364, 1105CrossRefGoogle Scholar
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