Larger sizes of massive quiescent early-type galaxies in clusters than in the field at 0.8 < z < 1.5

We analyse the mass–size relation of ∼400 quiescent massive ETGs (M */M⊙ > 3 × 1010) hosted by massive clusters (M200 ∼ 2–7 × 1014M⊙) at 0.8 

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2014-06, Vol.441 (1), p.203-223
Main Authors: Delaye, L., Huertas-Company, M., Mei, S., Lidman, C., Licitra, R., Newman, A., Raichoor, A., Shankar, F., Barrientos, F., Bernardi, M., Cerulo, P., Couch, W., Demarco, R., Muñoz, R., Sánchez-Janssen, R., Tanaka, M.
Format: Article
Language:English
Subjects:
Accretion disks
Cosmology
Evolution
Morphology
Sciences of the Universe
Star & galaxy formation
Universe
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Summary:We analyse the mass–size relation of ∼400 quiescent massive ETGs (M */M⊙ > 3 × 1010) hosted by massive clusters (M200 ∼ 2–7 × 1014M⊙) at 0.8 
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stu496