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...
| Main Authors: | , |
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| Other Authors: | , , |
| Format: | Article |
| Language: | English |
| Published: |
American Astronomical Society/IOP Publishing,
2018-03-20T13:40:30Z.
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| Subjects: | |
| Online Access: | Get fulltext |