A code comparison of the interaction between Milky Way disc and satellites
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...
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
02 August 2018
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| In: |
Proceedings of the International Astronomical Union
Year: 2017, Jahrgang: 13, Heft: S334, Pages: 339-340 |
| ISSN: | 1743-9221 |
| DOI: | 10.1017/S1743921317006482 |
| Online-Zugang: | Verlag, Volltext: https://doi.org/10.1017/S1743921317006482 Verlag, Volltext: https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/code-comparison-of-the-interaction-between-milky-way-disc-and-satellites/84862A3D68292A19E1949CBC4C1369CA 
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| Verfasserangaben: | Matteo Mazzarini and Andreas Just |
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| 520 | |a 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. | ||
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