The Evolution of Environmental Quenching Timescales to z ∼ 1.6: Evidence for Dynamically Driven Quenching of the Cluster Galaxy Population
R. Foltz, G. Wilson, A. Muzzin, M. C. Cooper, J. Nantais, R. F.J. Van Der Burg, P. Cerulo, J. Chan, S. P. Fillingham, J. Surace, T. Webb, A. Noble, M. Lacy, M. McDonald, G. Rudnick, C. Lidman, R. Demarco, J. Hlavacek-Larrondo, H. K.C. Yee, S. PerlmutterB. Hayden
Profundice en los temas de investigación de 'The Evolution of Environmental Quenching Timescales to z ∼ 1.6: Evidence for Dynamically Driven Quenching of the Cluster Galaxy Population'. En conjunto forman una huella única.