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- W1761501013 abstract "We suggest that the observed break in giant-planet frequency as a function of host metallicity at Z=0.02 may be a reflection of bimodal planet formation. We search for signatures of this bimodality in the distributions of the planet eccentricities, periods, masses, and multiplicity. However, the low-metallicity sample is at present too small to test for any but the most severe differences in these two putative populations." @default.
- W1761501013 created "2016-06-24" @default.
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- W1761501013 date "2003-12-11" @default.
- W1761501013 modified "2023-09-27" @default.
- W1761501013 title "Testing Bimodal Planet Formation" @default.
- W1761501013 hasPublicationYear "2003" @default.
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