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Erratum: "Unlocking CO Depletion in Protoplanetary Disks. I. The Warm Molecular Layer" (2018, ApJ, 856, 85)

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Published 2018 September 24 © 2018. The American Astronomical Society. All rights reserved.
, , Citation Kamber R. Schwarz et al 2018 ApJ 865 78 DOI 10.3847/1538-4357/aadfdf

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This is a correction for 2018 ApJ 856 85

0004-637X/865/1/78

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The model dust distribution reported in the published article is incorrect. The published article states that dust grains with the same height as the gas, referred to as small grains, have an MRN size distribution of rd = 0.005–1 μm, while the grains that are more settled than the gas, i.e., large grains, have a size distribution of rd = 0.005–1000 μm. The correct dust distribution is as follows: there are two populations of dust grains with the same scale height as the gas. Fifteen percent of these grains have an MRN size distribution of rd = 0.005–1 μm, the remaining 85% have a size distribution of rd = 0.005–1000 μm. The large-grain population, which is more settled than the gas, has a size distribution of rd = 10–1000 μm. The results and conclusions remain unchanged.

10.3847/1538-4357/aadfdf