The abundance of ultra-diffuse galaxies from groups to clusters. UDGs are relatively more common in more massive haloes

Author(s):: Burg, R.F.J. van der; Hoekstra, H. (0000-0001-7463-2893); Muzzin, A.; Sifón, C.; Viola, M.; Bremer, M.N.; Brough, S.; Driver, S.P.; Erben, T.; Heymans, C.; Hildebrandt, H.; Holwerda, B.W. (0000-0002-4884-6756); Klaes, D.; Kuijken, K.H. (0000-0002-3827-0175); McGee, S.L.; Nakajima, R.; Napolitano, N.; Norberg, P.; Taylor, E.N.; Valentijn, E.

Published: 2017
Publication type: Article / Letter to editor

Date issued: 2017
Language: English
Is part of: Astronomy & Astrophysics (0004-6361) (2017), Vol. 607, p. A79
hdl: 1887/59148
doi: 10.1051/0004-6361/201731335
URL: https://www.aanda.org/articles/aa/abs/2017/11/aa31335-17/aa31335-17.html