Simulations of MW-mass galaxies in the cosmological context
During the last three decades simulations of the formation of galaxies have made fantastic progress, overcoming problems such as the angular momentum catastrophe and producing galaxies that resemble disk-bulge systems similar to those observed. In this work, I discuss such progress focusing on the f...
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2017
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v13_nS334_p201_Scannapieco http://hdl.handle.net/20.500.12110/paper_17439213_v13_nS334_p201_Scannapieco |
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paper:paper_17439213_v13_nS334_p201_Scannapieco2023-06-08T16:27:57Z Simulations of MW-mass galaxies in the cosmological context cosmology: theory Galaxy: disk Galaxy: formation Galaxy: formation Galaxy: kinematics and dynamics methods: numerical During the last three decades simulations of the formation of galaxies have made fantastic progress, overcoming problems such as the angular momentum catastrophe and producing galaxies that resemble disk-bulge systems similar to those observed. In this work, I discuss such progress focusing on the formation and evolution of disks in galaxies similar to our Milky Way, and on the effects of different feedback processes that affect galaxies through cosmic time. I also present the results of simulations that use constrained initial conditions of the Local Group, and discuss environmental effects that might play a role in the formation and evolution of our Galaxy. © International Astronomical Union 2018. 2017 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v13_nS334_p201_Scannapieco http://hdl.handle.net/20.500.12110/paper_17439213_v13_nS334_p201_Scannapieco |
| institution |
Universidad de Buenos Aires |
| institution_str |
I-28 |
| repository_str |
R-134 |
| collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
| topic |
cosmology: theory Galaxy: disk Galaxy: formation Galaxy: formation Galaxy: kinematics and dynamics methods: numerical |
| spellingShingle |
cosmology: theory Galaxy: disk Galaxy: formation Galaxy: formation Galaxy: kinematics and dynamics methods: numerical Simulations of MW-mass galaxies in the cosmological context |
| topic_facet |
cosmology: theory Galaxy: disk Galaxy: formation Galaxy: formation Galaxy: kinematics and dynamics methods: numerical |
| description |
During the last three decades simulations of the formation of galaxies have made fantastic progress, overcoming problems such as the angular momentum catastrophe and producing galaxies that resemble disk-bulge systems similar to those observed. In this work, I discuss such progress focusing on the formation and evolution of disks in galaxies similar to our Milky Way, and on the effects of different feedback processes that affect galaxies through cosmic time. I also present the results of simulations that use constrained initial conditions of the Local Group, and discuss environmental effects that might play a role in the formation and evolution of our Galaxy. © International Astronomical Union 2018. |
| title |
Simulations of MW-mass galaxies in the cosmological context |
| title_short |
Simulations of MW-mass galaxies in the cosmological context |
| title_full |
Simulations of MW-mass galaxies in the cosmological context |
| title_fullStr |
Simulations of MW-mass galaxies in the cosmological context |
| title_full_unstemmed |
Simulations of MW-mass galaxies in the cosmological context |
| title_sort |
simulations of mw-mass galaxies in the cosmological context |
| publishDate |
2017 |
| url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v13_nS334_p201_Scannapieco http://hdl.handle.net/20.500.12110/paper_17439213_v13_nS334_p201_Scannapieco |
| _version_ |
1768545208707842048 |