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A code comparison of the interaction between Milky Way disc and satellites

Published online by Cambridge University Press:  02 August 2018

Matteo Mazzarini  and
Andreas Just
Matteo Mazzarini*
Affiliation:
Astronomisches Rechen-Institut, Zentrum für Astronomie Heidelberg, Heidelberg University, Mönchhofstr. 12-14, 69120 Heidelberg, Germany
Andreas Just
Affiliation:
Astronomisches Rechen-Institut, Zentrum für Astronomie Heidelberg, Heidelberg University, Mönchhofstr. 12-14, 69120 Heidelberg, Germany
*
1email: mazzarini@uni-heidelberg.de
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Abstract

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We present a comparison of previous simulations of the interaction of the Galactic disc with the Milky Way (MW) satellites using superbox-10 with new simulations performed with gadget-2 and ChaNGa. The robust performance of gadget-2 motivates us to employ more recent versions of gadget to identify the satellite debris in the MW halo, disc and bulge.

Keywords

methods: n-body simulationsGalaxy: discGalaxy: kinematics and dynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S334: Rediscovering our Galaxy , July 2017 , pp. 339 - 340
Copyright
Copyright © International Astronomical Union 2018 

Footnotes

†

Fellow of the International Max Planck Research School for Astronomy and Cosmic Physics at the University of Heidelberg (IMPRS-HD).

References

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