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Multilateral Study of the Andromeda Giant Stream: Implications for the progenitor, its MBH, and the M31 halo

Published online by Cambridge University Press:  21 March 2017

Takanobu Kirihara
Affiliation:
Faculty of Pure and Applied Physics, University of Tsukuba, Tennodai 1-1-1, Tsukuba, Japan email: [email protected]
Yohei Miki
Affiliation:
Center for Computational Sciences, University of Tsukuba, Tennodai 1-1-1, Tsukuba, Japan
Masao Mori
Affiliation:
Faculty of Pure and Applied Physics, University of Tsukuba, Tennodai 1-1-1, Tsukuba, Japan email: [email protected] Center for Computational Sciences, University of Tsukuba, Tennodai 1-1-1, Tsukuba, Japan
Toshihiro Kawaguchi
Affiliation:
Sapporo Medical University, S1W17, Chuoh-ku, Sapporo, Japan
R. Michael Rich
Affiliation:
Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA
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Abstract

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In a series of papers, we have performed N-body simulations of a galaxy collision to reproduce the observed shape, kinematics, and metallicity distribution of a giant stellar stream and shell-like structures in the halo of Andromeda galaxy (M31).

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2017 

References

Kawaguchi, T., Saito, Y., Miki, Y., & Mori, M. 2014, ApJ, 789, L13 Google Scholar
Kirihara, T., Miki, Y., & Mori, M. 2014, PASJ, 66, L10 Google Scholar
Kirihara, T., Miki, Y., Mori, M., & Kawaguchi, T. 2016, submitted to MNRAS, arXiv e-prints (arXiv:1603.02682)Google Scholar
Miki, Y., Mori, M., Kawaguchi, T., & Saito, Y. 2014, ApJ, 783, 87 CrossRefGoogle Scholar
Miki, Y., Mori, M., & Rich, M. R. 2016, in press, arXiv e-prints (arXiv:1606.03173)Google Scholar
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