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Dust and gas in luminous proto-cluster galaxies at z=4.05: the case for different cosmic dust evolution in normal and starburst galaxies

Abstract:

We measure the dust and gas content of the three submillimeter galaxies (SMGs) in the GN20 proto-cluster at z = 4.05 using new IRAM Plateau de Bure interferometer (PdBI) CO(4-3) and 1.2-3.3 mm continuum observations. All these three SMGs are heavily dust obscured, with UV-based star formation rate (SFR) estimates significantly smaller than the ones derived from the bolometric infrared (IR), consistent with the spatial offsets revealed by HST and CO imaging. Based also on evaluations of the sp...

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Publication status:
Published

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Publisher copy:
10.1051/0004-6361/201423905

Authors


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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
Publisher:
EDP Sciences
Journal:
ASTRONOMY and ASTROPHYSICS
Volume:
569
Pages:
A98-A98
Publication date:
2014-09-01
DOI:
EISSN:
1432-0746
ISSN:
0004-6361
Language:
English
Keywords:
Pubs id:
pubs:487023
UUID:
uuid:c79556b4-6d11-4c7c-9102-fd4fb6c13c1d
Local pid:
pubs:487023
Source identifiers:
487023
Deposit date:
2014-10-22

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