Modelling satellite galaxies in semi-analytical models

Understanding the evolution of satellite halos is important in predicting the abundance of dark matter subhalos and satellite galaxies. However, in numerical simulations of structure formation, spurious disruptions can occur that make the halos of some galaxies no longer detectable. Those galaxies t...

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Detalles Bibliográficos
Autores principales:	Delfino, F. M., Scóccola, Claudia Graciela, Vega Martínez, Cristian Antonio, Cora, Sofía Alejandra
Formato:	Articulo
Lenguaje:	Español
Publicado:	2021
Materias:	Ciencias Astronómicas galaxies: formation galaxies: evolution galaxies: halos methods: numerical
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/175994
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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