English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse
  1. View item / 
  2. Item Summary

Item

ITEM ACTIONSEXPORT
Add to Basket
  Local TagsRelease HistoryDetailsSummary

Released
Proceedings

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

MPS-Authors

Buck,  Tobias
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Macciò,  Andrea
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Ness,  Melissa
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Obreja,  Aura
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Dutton,  Aaron
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

External Resource

https://ui.adsabs.harvard.edu/abs/2018IAUS..334..209B
(Any fulltext)

Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)
There are no public fulltexts stored in PuRe
Supplementary Material (public)
There is no public supplementary material available
Citation

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


Cite as: https://hdl.handle.net/21.11116/0000-0005-CEA8-6
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.