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• W2024772602 startingPage "S531" @default.
• W2024772602 abstract "We report on the detection of the Rossiter–McLaughlin effect for the eccentric, super-Neptune exoplanet HAT-P-11b, based on radial-velocity measurements taken with the High Dispersion Spectrograph mounted on the Subaru 8.2 m telescope, and simultaneous photometry with the LCOGT 2.0 m Faulkes Telescope North, both located in Hawaii. The observed radial velocities during a planetary transit of HAT-P-11b show a persistent blue-shift, suggesting a spin–orbit misalignment in the system. The best-fit value for the projected spin–orbit misalignment angle is |${lambda}$||$=$| 103|$^circ$||$_{-18^circ}^{+22^circ}$|⁠. This fact suggests that not only hot-Jupiters, but also super-Neptunes like HAT-P-11b had once experienced dynamical processes, such as planet–planet scattering or Kozai migration." @default.
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• W2024772602 date "2011-03-25" @default.
• W2024772602 modified "2023-10-17" @default.
• W2024772602 title "A Possible Tilted Orbit of the Super-Neptune HAT-P-11b" @default.
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• W2024772602 doi "https://doi.org/10.1093/pasj/63.sp2.s531" @default.
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