[C ii] Emission in a Self-regulated Interstellar Medium
The [C ii ] 157.74 μ m fine-structure transition is one of the brightest and most well-studied emission lines in the far-infrared, produced in the interstellar medium (ISM) of galaxies. We study its properties in subparsec-resolution hydrodynamical simulations for an ISM patch with gas surface densi...
| मुख्य लेखकों: | , , , |
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| स्वरूप: | लेख |
| भाषा: | English |
| प्रकाशित: |
IOP Publishing
2024-01-01
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| श्रृंखला: | The Astrophysical Journal |
| विषय: | |
| ऑनलाइन पहुंच: | https://doi.org/10.3847/1538-4357/ad2eac |