Ram pressure profiles in galaxy groups and clusters

Using a hybrid method that combines non-radiative hydrodynamical simulations with a semianalytic model of galaxy formation, we determine the ram pressure experienced by galaxies in haloes with virial masses 12.5 ≤ log (M<sub>200</sub>/ h<sup>−1</sup> M⊙) < 15.35 as a funct...

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Detalles Bibliográficos
Autores principales:	Tecce, Tomás Enrique, Cora, Sofía Alejandra, Tissera, Patricia Beatriz
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2011
Materias:	Astronomía methods: numerical galaxies: clusters: general galaxies: clusters: intracluster medium galaxies: evolution galaxies: groups: general intergalactic medium
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/93549 http://mnras.oxfordjournals.org/content/416/4/3170 https://ri.conicet.gov.ar/handle/11336/9960
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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