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- W1520343903 abstract "The orbital elements of extreme mass ratio binaries will be modified by interactions with surrounding circumstellar disks. For brown dwarf companions to Solar-type stars the resulting orbital migration is sufficient to drive short period systems to merger, creating a brown dwarf desert at small separations. We highlight the similarities and the differences between the migration of brown dwarfs and massive extrasolar planets, and discuss how observations can test a migration model for the brown dwarf desert." @default.
- W1520343903 created "2016-06-24" @default.
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- W1520343903 date "2003-01-01" @default.
- W1520343903 modified "2023-09-26" @default.
- W1520343903 title "Orbital Migration and the Brown Dwarf Desert" @default.
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- W1520343903 doi "https://doi.org/10.1017/s0074180900210218" @default.
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