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The photometric method of extrasolar planet detection revisited

โœ Scribed by Alan Hale; Laurance R. Doyle


Publisher
Springer Netherlands
Year
1994
Tongue
English
Weight
667 KB
Volume
212
Category
Article
ISSN
0004-640X

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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