THE OCCURRENCE OF ADDITIONAL GIANT PLANETS INSIDE THE WATER–ICE LINE IN SYSTEMS WITH HOT JUPITERS: EVIDENCE AGAINST HIGH-ECCENTRICITY MIGRATION
The origin of Jupiter-mass planets with orbital periods of only a few days is still uncertain. It is widely believed that these planets formed near the water-ice line of the protoplanetary disk, and subsequently migrated into much smaller orbits. Most of the proposed migration mechanisms can be clas...
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American Astronomical Society/IOP Publishing
2018
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| Online Access: | http://hdl.handle.net/1721.1/114234 https://orcid.org/0000-0001-5761-6779 https://orcid.org/0000-0002-4265-047X |