The outcome of the protoplanetary disk o
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Amit Kashi; Noam Soker
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Article
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2011
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Elsevier Science
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English
β 339 KB
We suggest that planets, brown dwarfs, and even low mass stars can be formed by fragmentation of protoplanetary disks around very massive stars (M J 100 M ). We discuss how fragmentation conditions make the formation of very massive planetary systems around very massive stars favorable. Such planeta