Optically Thick [Oi] and [Cii] Emission toward NGC 6334A
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference43 articles.
1. The H+ region contribution to [C II] 158- m emission
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1. [C ii] 158 μm emission as an indicator of galaxy star formation rate;Monthly Notices of the Royal Astronomical Society;2023-12-11
2. Photodissociation and X-Ray-Dominated Regions;Annual Review of Astronomy and Astrophysics;2022-08-18
3. Probing Gas Kinematics and PDR Structure around O-type Stars in the Sh 2-305 H ii Region;The Astrophysical Journal;2021-12-01
4. The case for thermalization as a contributor to the [C ii] deficit;Monthly Notices of the Royal Astronomical Society;2021-02-20
5. Modeling Collisional Excitation of [O i] Fine Structure Line Emission from PDRs. I. Homogeneous Clouds;The Astrophysical Journal;2019-12-10
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