The bright end of the colour-magnitude relation of cluster galaxies

We investigate the physical processes involved in the development of the red sequence (RS) of cluster galaxies by using a combination of cosmological N-body simulations of clusters of galaxies and a semi-analytic model of galaxy formation. Results show good agreement between the general trend of the...

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Detalles Bibliográficos
Autores principales:	Jiménez, N., Cora, S.A., Bassino, L.P., Tecce, T.E., Smith Castelli, A.V.
Formato:	JOUR
Materias:	Galaxies: clusters: general Galaxies: elliptical and lenticular, cD Galaxies: evolution Galaxies: formation Galaxies: groups: general Galaxies: interactions
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00358711_v417_n1_p785_Jimenez
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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