Impact of Lyman alpha pressure on metal-poor dwarf galaxies
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Peer-reviewed
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Abstract
Understanding the origin of strong galactic outflows and the suppression of
star formation in dwarf galaxies is a key problem in galaxy formation. Using a
set of radiation-hydrodynamic simulations of an isolated dwarf galaxy embedded
in a
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1365-2966
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Science and Technology Facilities Council (ST/N000927/1)