Evolutionary paths among different red galaxy types at 0.3 < z < 1.5 and the late buildup of massive E-S0s through major mergers-Reference-Cited by-同舟云学术

Evolutionary paths among different red galaxy types at 0.3 < z < 1.5 and the late buildup of massive E-S0s through major mergers

Published:2012-10-26 Issue:2 Volume:428 Page:999-1019
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Prieto M.,Eliche-Moral M. C.,Balcells M.,Cristobal-Hornillos D.,Erwin P.,Abreu D.,Dominguez-Palmero L.,Hempel A.,Lopez-Sanjuan C.,Guzman R.,Perez-Gonzalez P. G.,Barro G.,Gallego J.,Zamorano J.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/428/2/999/3192869/sts065.pdf

Reference162 articles.

1. Near‐Infrared and Star‐forming Properties of Local Luminous Infrared Galaxies

2. Measuring the fading of S0 galaxies using globular clusters

3. The SWIRE-VVDS-CFHTLS surveys: stellar mass assembly over the last 10 Gyr. Evidence for a major build up of the red sequence betweenz= 2 andz= 1

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