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: | Kannan, Rahul, Marinacci, Federico, Vogelsberger, Mark, Sales, Laura V, Torrey, Paul, Springel, Volker, Hernquist, Lars |
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Other Authors: | MIT Kavli Institute for Astrophysics and Space Research |
Format: | Article |
Language: | English |
Published: |
Oxford University Press (OUP)
2021
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Online Access: | https://hdl.handle.net/1721.1/130342 |
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