An Imperfectly Passive Nature: Bright Submillimeter Emission from Dust-obscured Star Formation in the z = 3.717 “Passive” System, ZF 20115-Reference-Cited by-同舟云学术

An Imperfectly Passive Nature: Bright Submillimeter Emission from Dust-obscured Star Formation in the z = 3.717 “Passive” System, ZF 20115

Published:2017-07-19 Issue:1 Volume:844 Page:L10
ISSN:2041-8213
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Simpson J. M.^ORCID,Smail Ian^ORCID,Wang Wei-Hao^ORCID,Riechers D.^ORCID,Dunlop J. S.,Ao Y.^ORCID,Bourne N.,Bunker A.,Chapman S. C.,Chen Chian-Chou^ORCID,Dannerbauer H.^ORCID,Geach J. E.,Goto T.,Harrison C. M.^ORCID,Hwang H. S.^ORCID,Ivison R. J.,Kodama Tadayuki^ORCID,Lee C.-H.,Lee H.-M.,Lee M.^ORCID,Lim C.-F.,Michałowski M. J.,Rosario D. J.^ORCID,Shim H.,Shu X. W.^ORCID,Swinbank A. M.^ORCID,Tee W.-L.,Toba Y.^ORCID,Valiante E.,Wang Junxian,Zheng X. Z.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/2041-8213/aa7cf2/pdf

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