Ram pressure profiles in galaxy groups and clusters

Using a hybrid method that combines non-radiative hydrodynamical simulations with a semi-analytic model of galaxy formation, we determine the ram pressure experienced by galaxies in haloes with virial masses 12.5 ≤ log(M 200/h -1M ⊙) < 15.35 as a function of the halocentric distance, for reds...

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Detalles Bibliográficos
Publicado:	2011
Materias:	Galaxies: clusters: general Galaxies: clusters: intracluster medium Galaxies: evolution Galaxies: groups: general Intergalactic medium Methods: numerical
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v416_n4_p3170_Tecce http://hdl.handle.net/20.500.12110/paper_00358711_v416_n4_p3170_Tecce
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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