Predicting Quiescence: The Dependence of Specific Star Formation Rate on Galaxy Size and Central Density at 0.5

Published:2017-03-20 Issue:1 Volume:838 Page:19
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Whitaker Katherine E.^ORCID,Bezanson Rachel^ORCID,van Dokkum Pieter G.^ORCID,Franx Marijn^ORCID,van der Wel Arjen^ORCID,Brammer Gabriel^ORCID,Förster-Schreiber Natascha M.^ORCID,Giavalisco Mauro^ORCID,Labbé Ivo^ORCID,Momcheva Ivelina G.^ORCID,Nelson Erica J.^ORCID,Skelton Rosalind^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/838/i=1/a=19/pdf

Reference114 articles.

1. CANDELS: THE PROGENITORS OF COMPACT QUIESCENT GALAXIES ATz∼ 2

2. SUB-KILOPARSEC ALMA IMAGING OF COMPACT STAR-FORMING GALAXIES AT z ∼ 2.5: REVEALING THE FORMATION OF DENSE GALACTIC CORES IN THE PROGENITORS OF COMPACT QUIESCENT GALAXIES

3. WHAT TURNS GALAXIES OFF? THE DIFFERENT MORPHOLOGIES OF STAR-FORMING AND QUIESCENT GALAXIES SINCEz∼ 2 FROM CANDELS

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