@WASPplanets @decaelus Stellar evolution models suggest that tidal dissipation due to a hot Jupiter should change dramatically over time (1e3 < Q < 1e8; Bolmont & Mathis 2016, https://t.co/2UDJiVjw7q, Fig. 1b, dashed lines). What do Q measurement
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"Effect of the rotation and tidal dissipation history of stars on the evolution of close-in planets" See https://t.co/iCq0LbpJcx
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RT @AstroPHYPapers: Effect of the rotation and tidal dissipation history of stars on the evolution of close-in planets. https://t.co/RfPyFh…
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Effect of the rotation and tidal dissipation history of stars on the evolution of close-in planets. https://t.co/RfPyFh2yxO
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Effect of the rotation and tidal dissipation history of stars on the evolution of close-in planets https://t.co/GJZwveZMbr