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- W1635016768 abstract "The dust around young stellar objects is supposed to be blown out or processed very quickly compared to the stellar lifetime. Nevertheless, large amounts of dust have been detected around s Pictoris and many other main sequence (MS) stars, according to their IR excess. The study of the evolutionary status, origin and lifetime of such environment is related to scenarii of star and planetary system formation, but it is still very poorly observationally constrained. Recent improvements in observational techniques, with the ESO adaptive optics system and a coronograph, allow further investigations of the s Pictoris disk and the characterization of the dust around other MS stars." @default.
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- W1635016768 date "1996-01-01" @default.
- W1635016768 modified "2023-09-25" @default.
- W1635016768 title "Coronographic Search for Dust Around Main Sequence Stars" @default.
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- W1635016768 doi "https://doi.org/10.1007/978-3-540-68594-4_42" @default.
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