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- W3102113748 endingPage "32" @default.
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- W3102113748 abstract "A crucial aspect of understanding planet formation is determining the binarity of the host stars. Results from radial velocity surveys and the follow-up of Kepler exoplanet candidates have demonstrated that stellar binarity certainly does not exclude the presence of planets in stable orbits and the configuration may in fact be relatively common. Here we present new results for the 30 Arietis system which confirms that the B component hosts both planetary and stellar companions. Keck AO imaging provides direct detection of the stellar companion and additional radial velocity data are consistent with an orbiting star. We present a revised orbit of the known planet along with photometry during predicted transit times. Finally, we provide constraints on the properties of the stellar companion based on orbital stability considerations." @default.
- W3102113748 created "2020-11-23" @default.
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- W3102113748 date "2015-12-03" @default.
- W3102113748 modified "2023-10-11" @default.
- W3102113748 title "ON THE STELLAR COMPANION TO THE EXOPLANET HOSTING STAR 30 ARIETIS B" @default.
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- W3102113748 doi "https://doi.org/10.1088/0004-637x/815/1/32" @default.
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