Dust formation in Milky Way-like galaxies
We introduce a dust model for cosmological simulations implemented in the moving-mesh code arepo and present a suite of cosmological hydrodynamical zoom-in simulations to study dust formation within galactic haloes. Our model accounts for the stellar production of dust, accretion of gas-phase metals...
| Main Authors: | , , , , |
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| Other Authors: | |
| Format: | Article |
| Language: | en_US |
| Published: |
Oxford University Press
2017
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| Online Access: | http://hdl.handle.net/1721.1/108526 https://orcid.org/0000-0001-9018-1180 https://orcid.org/0000-0001-8593-7692 https://orcid.org/0000-0002-5653-0786 |