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  NIHAO-UHD: High-resolution Simulations of MW mass galaxies

Buck, T., Macciò, A., Ness, M., Obreja, A., & Dutton, A. (2018). NIHAO-UHD: High-resolution Simulations of MW mass galaxies.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0005-CEA8-6 Version Permalink: https://hdl.handle.net/21.11116/0000-0005-CEA9-5
Genre: Proceedings

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https://ui.adsabs.harvard.edu/abs/2018IAUS..334..209B (Any fulltext)
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 Creators:
Buck, Tobias1, Author
Macciò, Andrea1, Author
Ness, Melissa1, Author
Obreja, Aura1, Author
Dutton, Aaron1, Author
Affiliations:
1Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners, ou_2421692              

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Free keywords: Galaxy: bulge Galaxy: evolution Galaxy: formation Galaxy: kinematics and dynamics Galaxy: structure Galaxy: center methods: numerical
 Abstract: High resolution cosmological and hydrodynamical simulations have reached a resolution able to resolve in a self consistent way the disc of our galaxy, the galaxy center and the satellites orbiting around it. We present first results from the NIHAO-UHD project, a set of very high- resolution baryonic zoom-in simulations of Milky Way mass disc galaxies. These simulations model the full cosmological assembly history of the galaxies and their satellite system using the same, well tested physics as the NIHAO project. We show that these simulations can self- consistently reproduce the observed kinematical and morphological features of the X-shaped bulge observed in our own Milky Way.

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 Dates: 2018
 Publication Status: Issued
 Pages: 209-212
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: -
 Degree: -

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Title: Rediscovering Our Galaxy
Place of Event: -
Start-/End Date: 2018

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