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Properties of Interstellar Medium in Star-Forming Galaxies at z~1.4 revealed with ALMA

Abstract:

We conducted observations of 12CO(J = 5-4) and dust thermal continuum emission toward 20 star-forming galaxies on the main sequence at z ∼ 1.4 using ALMA to investigate the properties of the interstellar medium. The sample galaxies are chosen to trace the distributions of star-forming galaxies in diagrams of stellar mass versus star formation rate and stellar mass versus metallicity. We detected CO emission lines from 11 galaxies. The molecular gas mass is derived by adopting a metallicity-de...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's version

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Publisher copy:
10.3847/0004-637X/819/1/82

Authors


Hatsukade, B More by this author
Akiyama, M More by this author
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Publisher:
IOP Publishing Publisher's website
Journal:
The Astrophysical Journal Journal website
Volume:
819
Issue:
1
Pages:
82-82
Publication date:
2016-03-01
DOI:
EISSN:
1538-4357
ISSN:
0004-637X
URN:
uuid:28de560a-05c9-4c53-9fa4-b5f27583cea5
Source identifiers:
578885
Local pid:
pubs:578885

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