Morphology and the color-mass diagram as clues to galaxy evolution at z∼1

Powell, Meredith C. and Urry, C. Megan and Cardamone, Carolin N. and Simmons, Brooke D. and Schawinski, Kevin and Young, Sydney and Kawakatsu, Mari (2017) Morphology and the color-mass diagram as clues to galaxy evolution at z∼1. The Astrophysical Journal, 835 (1). ISSN 0004-637X

[img]
Preview
PDF (accepted version)
accepted_version.pdf - Accepted Version
Available under License Creative Commons Attribution.

Download (2MB)

Abstract

We study the significance of mergers in the quenching of star formation in galaxies at z ~ 1 by examining their color–mass distributions for different morphology types. We perform two-dimensional light profile fits to GOODS iz images of ~5000 galaxies and X-ray selected active galactic nucleus (AGN) hosts in the CANDELS/GOODS-north and south fields in the redshift range 0.7<z<1.3. Distinguishing between bulge-dominated and disk-dominated morphologies, we find that disks and spheroids have distinct color–mass distributions, in agreement with studies at z ~ 0. The smooth distribution across colors for the disk galaxies corresponds to a slow exhaustion of gas, with no fast quenching event. Meanwhile, blue spheroids most likely come from major mergers of star-forming disk galaxies, and the dearth of spheroids at intermediate green colors is suggestive of rapid quenching. The distribution of moderate luminosity X-ray AGN hosts is even across colors, in contrast, and we find similar numbers and distributions among the two morphology types with no apparent dependence on Eddington ratio. The high fraction of bulge-dominated galaxies that host an AGN in the blue cloud and green valley is consistent with the scenario in which the AGN is triggered after a major merger, and the host galaxy then quickly evolves into the green valley. This suggests AGN feedback may play a role in the quenching of star formation in the minority of galaxies that undergo major mergers.

Item Type:
Journal Article
Journal or Publication Title:
The Astrophysical Journal
Additional Information:
This is an author-created, un-copyedited version of an article accepted for publication/published in The Astrophysical Journal. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it.
Uncontrolled Keywords:
/dk/atira/pure/subjectarea/asjc/1900/1912
Subjects:
ID Code:
127623
Deposited By:
Deposited On:
20 Sep 2018 10:14
Refereed?:
Yes
Published?:
Published
Last Modified:
23 Sep 2020 04:36