Simulating the interstellar medium of galaxies with radiative transfer, non-equilibrium thermochemistry, and dust
We present a novel framework to self-consistently model the effects of radiation fields, dust physics, and molecular chemistry (H2) in the interstellar medium (ISM) of galaxies. The model combines a state-of-the-art radiation hydrodynamics module with a H and He non-equilibrium thermochemistry mod...
| Main Authors: | , , , , , , |
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| Other Authors: | , |
| Format: | Article |
| Language: | English |
| Published: |
Oxford University Press (OUP),
2021-04-01T20:23:36Z.
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| Subjects: | |
| Online Access: | Get fulltext |