Molecular gas, stars, and dust in sub-L super() star-forming galaxies at z ~ 2: Evidence for univers...
Molecular gas, stars, and dust in sub-L super() star-forming galaxies at z ~ 2: Evidence for universal star formation and non-universal dust-to-gas ratio
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English
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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 sub(*)). It is yet essential to extend the CO measurements to the more numerous z ~ 2 SFGs with L sub(IR) < L super() = 4 10 super(11) L sub() and M sub(*) < 2.5 10 super(10) M sub(). We have achiev...
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Molecular gas, stars, and dust in sub-L super() 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_miscellaneous_1893892193
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1893892193
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ISSN
1743-9213
E-ISSN
1743-9221
DOI
10.1017/S1743921316007584
