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• W1623409879 abstract "Abstract The star β Pictoris is not in itself very remarkable; however, it is surrounded by a dust disk that is much more prominent than any other main sequence star’s disk. The proximity of β Pic and the nearly edge-on viewing geometry of the disk enhance its appearance, but do not fully account for the disk’s prominence. While it is possible that β Pic’s disk is intrinsically unusual, a more likely explanation is that β Pic is simply a very young (~ 20 Myr old) main sequence star with a consequently denser second-generation debris disk remnant of its protostellar disk than possessed by older main sequence A stars." @default.
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• W1623409879 date "2002-01-01" @default.
• W1623409879 modified "2023-10-16" @default.
• W1623409879 title "The β Pictoris Disk: Peculiar or Just Young?" @default.
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• W1623409879 doi "https://doi.org/10.1017/s0252921100001548" @default.
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