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- W3100478710 abstract "The dwarf galaxy companions to the Milky Way are unique cosmological laboratories. With luminosities as low as<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML><mml:mrow><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mo>−</mml:mo><mml:mn>7</mml:mn></mml:mrow></mml:msup><mml:msub><mml:mi>L</mml:mi><mml:mrow><mml:mtext>MW</mml:mtext></mml:mrow></mml:msub></mml:mrow></mml:math>, they inhabit the lowest mass dark matter halos known to host stars and are presently the most direct tracers of the distribution, mass spectrum, and clustering scale of dark matter. Their resolved stellar populations also facilitate detailed studies of their history and mass content. To fully exploit this potential requires a well-defined census of virtually invisible galaxies to the faintest possible limits and to the largest possible distances. I review the past and present impacts of survey astronomy on the census of Milky Way dwarf galaxy companions and discuss the future of finding ultra-faint dwarf galaxies around the Milky Way and beyond in wide-field survey data." @default.
- W3100478710 created "2020-11-23" @default.
- W3100478710 creator A5039451774 @default.
- W3100478710 date "2010-01-01" @default.
- W3100478710 modified "2023-09-26" @default.
- W3100478710 title "In Pursuit of the Least Luminous Galaxies" @default.
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- W3100478710 doi "https://doi.org/10.1155/2010/285454" @default.
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