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The ALMaQUEST Survey: III. Scatter in the resolved star forming main sequence is primarily due to variations in star formation efficiency
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cited authors
Ellison, Sara L; Thorp, Mallory D; Lin, Lihwai; Pan, Hsi-An; Bluck, Asa FL; Scudder, Jillian M; Teimoorinia, Hossen; Sanchez, Sebastian F; Sargent, Mark
authors
Bluck, Asa
publication date
November 26, 2019
webpage
http://dx.doi.org/10.1093/mnrasl/slz179
http://arxiv.org/abs/1911.11887v1
Research
keywords
astro-ph.GA