The temporal evolution of gas accretion onto the discs of simulated Milky Way-mass galaxies

En el modelo estándar de formación de estructura, las galaxias se forman en los centros de los halos de materia oscura que surgen como resultado de inhomogeneidades en la distribución primodial de masa del Universo. Posteriormente, las galaxias crecen mediante la acreción continua de material gaseos...

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Detalles Bibliográficos
Autores principales:	Iza, Federico, Nuza, Sebastián Ernesto, Scannapieco, Cecilia
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2023
Materias:	Ciencias Astronómicas galaxies: evolution galaxies: structure methods: numerical
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/164360
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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