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• W2558388889 startingPage "L6" @default.
• W2558388889 abstract "We present subarcsecond images of submillimeter CO and continuum emission from a local galaxy forming massive star clusters: the blue compact dwarf galaxy II Zw 40. At $sim$0.4 resolution (20 pc), the CO(3-2), CO(1-0), 3mm and 870${mu}$m continuum maps illustrate star formation on the scales of individual molecular clouds. Dust contributes about a third of the 870${mu}$m continuum emission, with free-free accounting for the rest. On these scales, there is not a good correspondence between gas, dust, and free-free emission. Dust continuum is enhanced toward the star-forming region as compared to the CO emission. We suggest that an unexpectedly low and spatially variable gas-to-dust ratio is the result of massive clusters of the starburst." @default.
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• W2558388889 date "2016-12-01" @default.
• W2558388889 modified "2023-09-27" @default.
• W2558388889 title "ALMA REVEALS POTENTIAL LOCALIZED DUST ENRICHMENT FROM MASSIVE STAR CLUSTERS IN II Zw 40" @default.
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• W2558388889 doi "https://doi.org/10.3847/2041-8205/833/1/l6" @default.
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