Is the cluster environment quenching the Seyfert activity in elliptical and spiral galaxies?

Is the cluster environment quenching the Seyfert activity in elliptical and spiral galaxies?

We developed a hierarchical Bayesian model (HBM) to investigate how the presence of Seyfert activity relates to their environment, herein represented by the galaxy cluster mass, M200, and the normalized cluster centric distance, r/r200. We achieved this by constructing an unbiased sample of galaxies...

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Bibliographic Details
Main Authors:	de Souza, R, Dantas, M, Krone-Martins, A, Cameron, E, Coelho, P, Hattab, M, de Val-Borro, M, Hilbe, J, Elliott, J, Hagen, A
Format:	Journal article
Published:	Oxford University Press 2016

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