Modeling gas-phase H2O between 5 $\mathsf{\mu}$m and 540 $\mathsf{\mu}$m toward massive protostars
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20030765/pdf
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1. Water Abundance and Velocity Structure in S140, ρ Oph A, and B335
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