Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 ≤z< 3-Reference-Cited by-同舟云学术

Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 ≤z< 3

Published:2018-01-26 Issue:2 Volume:853 Page:108
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Guo Yicheng^ORCID,Rafelski Marc^ORCID,Bell Eric F.^ORCID,Conselice Christopher J.^ORCID,Dekel Avishai^ORCID,Faber S. M.,Giavalisco Mauro^ORCID,Koekemoer Anton M.^ORCID,Koo David C.^ORCID,Lu Yu^ORCID,Mandelker Nir^ORCID,Primack Joel R.^ORCID,Ceverino Daniel^ORCID,de Mello Duilia F.^ORCID,Ferguson Henry C.^ORCID,Hathi Nimish^ORCID,Kocevski Dale,Lucas Ray A.^ORCID,Pérez-González Pablo G.,Ravindranath Swara,Soto Emmaris^ORCID,Straughn Amber,Wang Weichen

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/853/i=2/a=108/pdf

Reference122 articles.

1. Structural and Star-forming Relations sincez∼ 3: Connecting Compact Star-forming and Quiescent Galaxies

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. DYNAMO – II. Coupled stellar and ionized-gas kinematics in two low-redshift clumpy discs

4. THE ROLE OF BULGE FORMATION IN THE HOMOGENIZATION OF STELLAR POPULATIONS ATZ∼ 2 AS REVEALED BY INTERNAL COLOR DISPERSION IN CANDELS

5. The stellar masses of 25 000 galaxies at 0.2 ≤ z ≤ 1.0 estimated by the COMBO-17 survey

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