Models of the in Situ Formation of Detec
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Peter Bodenheimer; Olenka Hubickyj; Jack J. Lissauer
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Article
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2000
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Elsevier Science
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English
โ 138 KB
We present numerical simulations of the formation of the planetary companions to 47 UMa, ฯ CrB, and 51 Peg. They are assumed to have formed in situ according to the basic model that a core formed first by accretion of solid particles, then later it captured substantial amounts of gas from the protop