Molecular gas, stars, and dust in sub-L ⋆ star-forming galaxies at z ~ 2: Evidence for universal sta...
Molecular gas, stars, and dust in sub-L ⋆ star-forming galaxies at z ~ 2: Evidence for universal star formation and non-universal dust-to-gas ratio
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Publisher
Cambridge, UK: Cambridge University Press
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Language
English
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Publisher
Cambridge, UK: Cambridge University Press
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Contents
Current star-forming galaxies (SFGs) with CO measurements at z ~ 2 suffer from a bias toward high star formation rates (SFR) and high stellar masses (M
*). It is yet essential to extend the CO measurements to the more numerous z ~ 2 SFGs with L
IR < L
⋆ = 4× 1011 L⊙ and M
* < 2.5× 1010 M⊙. We have achieved CO, stars, and dust measuremen...
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Full title
Molecular gas, stars, and dust in sub-L ⋆ star-forming galaxies at z ~ 2: Evidence for universal star formation and non-universal dust-to-gas ratio
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TN_cdi_proquest_journals_1871156443
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_1871156443
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ISSN
1743-9213
E-ISSN
1743-9221
DOI
10.1017/S1743921316007584