TY  - JOUR
AU  - Zarattini, S.
AU  - Barrena, R.
AU  - Girardi, M.
AU  - Castro Rodríguez, N.
AU  - Boschin, W.
AU  - Aguerri, J. A. L.
AU  - Mendéz Abreu, J.
AU  - Sánchez Janssen, R.
AU  - Catalán Torrecilla, Cristina
AU  - Corsini, E. M.
AU  - Burgo, C. del
AU  - D'Onghia, E.
AU  - Herrera Ruiz, N.
AU  - Iglesias Páramo, J.
AU  - Jiménez Bailón, E.
AU  - Lozada Muñoz, M.
AU  - Napolitano, N.
AU  - Vilchez, J. M.
PY  - 2014
DO  - 10.1051/0004-6361/201323351
SN  - 0004-6361
UR  - https://hdl.handle.net/20.500.14352/33763
T2  - Astronomy & Astrophysics
AB  - Context. Virialized halos grow by the accretion of smaller ones in the cold dark matter scenario. The rate of accretion depends on the different properties of the host halo. Those halos for which this accretion rate was very fast and efficient...
LA  - eng
PB  - EDP Sciencies
KW  - Digital Sky Survey
KW  - Galaxy-Cluster-Survey
KW  - X-Ray Luminosity
KW  - Brightest Group Galaxies
KW  - Velocity Dispersions
KW  - Millennium Simulation
KW  - Internal Dynamics
KW  - Scaling Relations
KW  - Redshift Survey
KW  - Stellar Mass
TI  - Fossil group origins IV. Characterization of the sample and observational properties of fossil systems
TY  - journal article
VL  - 565
ER  -