Herschel 158 μm [C ii] Observations of “CO-dark” Gas in the Perseus Giant Molecular Cloud
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab9b86/pdf
Reference99 articles.
1. Radiative transfer meets Bayesian statistics: where does a galaxy's [C ii] emission come from?
2. From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from theHerschelGould Belt Survey
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1. CO and [C ii] line emission of molecular clouds: the impact of stellar feedback and non-equilibrium chemistry;Monthly Notices of the Royal Astronomical Society;2023-09-01
2. On the Three-dimensional Structure of Local Molecular Clouds;The Astrophysical Journal;2021-09-01
3. Massive molecular gas reservoir around the central AGN in the CARLA J1103 + 3449 cluster at z = 1.44;Astronomy & Astrophysics;2020-09
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