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- W106593279 abstract "Ultra faint dwarf spheroidal galaxies (UFs) are the least luminous and the least metal-rich stellar systems ever known (L 105Ls un) dwarf spheroidal galaxies (dSphs), suggesting that the formation of all these Milky Way (MW) satellites has been governed by the same physical processes. However while classical dSphs and UFs together span more than four orders of magnitude in luminosity, their total mass is roughly the same within the innermost 300 pc. Why is then the star formation so inefficient in UFs? Moreover recent observations of metal-poor stars in dSphs have revealed that [F e/H] 8.5, i.e. before the reionization epoch." @default.
- W106593279 created "2016-06-24" @default.
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- W106593279 date "2010-01-01" @default.
- W106593279 modified "2023-09-26" @default.
- W106593279 title "Probing the High Redshift Universe with the faintest dwarfs" @default.
- W106593279 hasPublicationYear "2010" @default.
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