Alma maging of the co (7−6) line emission in the submillimeter galaxy less 073 at z = 4.755
In this paper we present our imaging observations on the CO (7−6) line and its underlying continuum emission of the young submillimeter galaxy LESS 073 at redshift 4.755, using the Atacama Large Millimeter/submillimeter Array (ALMA). At the achieved resolution of ∼1 ′′ .2 × 0 ′′ .9 (8 × 6 kpc2 ), the CO (7−6) emission is largely unresolved (with a deconvolved size of 1′′ .1(±0 ′′ .5) × 0 ′′ .9(±0 ′′ .8).), and the continuum emission is totally unresolved. The CO (7−6) line emission has an int...Expand abstract
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- American Astronomical Society.
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- This is the accepted manuscript version of the article. The final version is available from American Astronomical Society at: https://doi.org/10.3847/1538-4357/ab75eb
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