The Occurrence of Additional Giant Planets Inside the Water-Ice Line in Systems with Hot Jupiters: Evidence Against High-Eccentricity Migration

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Schlaufman, Kevin C.; Winn, Joshua N.; (2016)
  • Related identifiers: doi: 10.3847/0004-637X/825/1/62
  • Subject: Astrophysics - Solar and Stellar Astrophysics | Astrophysics - Earth and Planetary Astrophysics
    arxiv: Astrophysics::Earth and Planetary Astrophysics | Astrophysics::Solar and Stellar Astrophysics

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 mi... View more
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