Galaxy Merger Candidates in High-redshift Cluster Environments-Reference-Cited by-同舟云学术

Galaxy Merger Candidates in High-redshift Cluster Environments

Published:2017-07-12 Issue:2 Volume:843 Page:126
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Delahaye A. G.,Webb T. M. A.,Nantais J.,DeGroot A.,Wilson G.,Muzzin A.^ORCID,Yee H. K. C.,Foltz R.,Noble A. G.^ORCID,Demarco R.,Tudorica A.,Cooper M. C.^ORCID,Lidman C.^ORCID,Perlmutter S.,Hayden B.^ORCID,Boone K.,Surace J.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/843/i=2/a=126/pdf

Reference71 articles.

1. THE ENVIRONMENTAL DEPENDENCE OF THE INCIDENCE OF GALACTIC TIDAL FEATURES

2. The evolution of dust-obscured star formation activity in galaxy clusters relative to the field over the last 9 billion years★

3. Observational evidence that massive cluster galaxies were forming stars atz~ 2.5 and did not grow in mass at later times

4. The insignificant evolution of the richness-mass relation of galaxy clusters

5. Star formation quenching in simulated group and cluster galaxies: when, how, and why?

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