High-resolution three-dimensional simulations of gas removal from ultrafaint dwarf galaxies I. Stellar feedback
Context. The faintest Local Group galaxies found lurking in and around the Milky Way halo provide a unique test bed for theories of structure formation and evolution on small scales. Deep Subaru and Hubble Space Telescope photometry demonstrates that the stellar populations of these galaxies are old...
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Published in | Astronomy and astrophysics (Berlin) Vol. 630; p. A140 |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
01.10.2019
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Online Access | Get full text |
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