On the formation of planetary systems in photoevaporating transition discs
In protoplanetary discs, planetary cores must be at least 0.1 M⊕ at 1 au for migration to be significant; this mass rises to 1 M⊕ at 5 au. Planet formation models indicate that these cores form on million year time-scales. We report here a study of the evolution of 0.1 and 1 M⊕ cores, migrating from...
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| বিন্যাস: | Journal article |
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Oxford University Press
2016
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