Evolución químico-dinámica de galaxias masivas en contexto cosmológico

En este trabajo, analizamos la Relación Masa-Metalicidad de galaxias con el conjunto de simulaciones EAGLE, focalizándonos en galaxias de masa estelar mayor a 10¹⁰ M☉. Nuestros resultados muestran que, a masa fija, la metalicidad del gas tiende a decrecer con la fracción de gas de la galaxia, especi...

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Detalles Bibliográficos
Autores principales:	Santamaria, Ramiro, De Rossi, M.E., Zenocratti, Lucas José
Formato:	Articulo
Lenguaje:	Español
Publicado:	2022
Materias:	Ciencias Astronómicas galaxies: formation galaxies: evolution galaxies: abundances galaxies: star formation cosmology: theory
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/168604
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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