@Article{SampaioCaFeLaRiRe:2021:InPrPh,
               author = "Sampaio, Vitor Medeiros and Carvalho, R. R. de and Ferrera, I. and 
                         Lagana, T. F. and Ribeiro, A. L. B. and Rembold, S. B.",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and 
                         {Universidade Cruzeiro do Sul} and {Instituto de 
                         Astrof{\'{\i}}sica de Canarias} and {Universidade Cruzeiro do 
                         Sul} and {Universidade Estadual de Santa Cruz} and {Universidade 
                         Federal de Santa Maria (UFSM)}",
                title = "Investigating the projected phase space of Gaussian and 
                         non-Gaussian clusters",
              journal = "Monthly Notices of the Royal Astronomical Society",
                 year = "2021",
               volume = "503",
               number = "2",
                pages = "3065--3080",
                month = "May",
             keywords = "galaxies: clusters: general, galaxy: evolution, galaxy: 
                         formation.",
             abstract = "By way of the projected phase space (PPS), we investigate the 
                         relation between galaxy properties and cluster environment in a 
                         subsample of groups from the Yang catalogue. The sample is split 
                         according to the Gaussianity of the velocity distribution in the 
                         group into Gaussian (G) and non-Gaussian (NG). Our sample is 
                         limited to massive clusters with M-200 >= 10(14) M-circle dot and 
                         0.03 <= z <= 0.1. NG clusters are more massive, less concentrated 
                         and have an excess of faint (F) galaxies compared to G clusters. 
                         NG clusters show mixed distributions of galaxy properties in the 
                         PPS compared to the G case. Using the relation between infall time 
                         and locus on the PPS, we find that, on average, NG clusters 
                         accreted similar to 10(11) M-circle dot more stellar mass in the 
                         last similar to 5 Gyr than G clusters. The relation between galaxy 
                         properties and infall time is significantly different for galaxies 
                         in G and NG systems. The more mixed distribution in the PPS of NG 
                         clusters translates into shallower relations with infall time. F 
                         galaxies whose first crossing of the cluster virial radius 
                         happened 2-4 Gyr ago in NG clusters are older and more metal-rich 
                         than in G systems. All these results suggest that NG clusters 
                         experience a higher accretion of pre-processed galaxies, which 
                         characterizes G and NG clusters as different environments to study 
                         galaxy evolution.",
                  doi = "10.1093/mnras/stab673",
                  url = "http://dx.doi.org/10.1093/mnras/stab673",
                 issn = "0035-8711 and 1365-2966",
             language = "en",
           targetfile = "sampaio_investigating.pdf",
        urlaccessdate = "29 jun. 2024"
}