ORBITAL STABILITY OF MULTI-PLANET SYSTEMS: BEHAVIOR AT HIGH MASSES
In the coming years, high-contrast imaging surveys are expected to reveal the characteristics of the population of wide-orbit, massive, exoplanets. To date, a handful of wide planetary mass companions are known, but only one such multi-planet system has been discovered: HR 8799. For low mass planeta...
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| Language: | en |
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IOP PUBLISHING LTD
2016
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| Online Access: | http://hdl.handle.net/10150/621257 http://arizona.openrepository.com/arizona/handle/10150/621257 |