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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Detalles Bibliográficos
Autor principal: Scannapieco, C.
Formato: SER
Materias:
cosmology: theory
Galaxy: disk
Galaxy: formation
Galaxy: kinematics and dynamics
methods: numerical
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_17439213_v13_nS334_p201_Scannapieco
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id todo:paper_17439213_v13_nS334_p201_Scannapieco
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spelling todo:paper_17439213_v13_nS334_p201_Scannapieco2023-10-03T16:31:28Z Simulations of MW-mass galaxies in the cosmological context Scannapieco, C. 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. SER info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar 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
Scannapieco, C.
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.
format SER
author Scannapieco, C.
author_facet Scannapieco, C.
author_sort Scannapieco, C.
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
url http://hdl.handle.net/20.500.12110/paper_17439213_v13_nS334_p201_Scannapieco
work_keys_str_mv AT scannapiecoc simulationsofmwmassgalaxiesinthecosmologicalcontext
_version_ 1807317515561336832

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