Add to ORKGWe present spectroscopy of a transit of the exoplanet HD 189733b. By modeling the Rossiter-McLaughlin effect (the anomalous Doppler shift due to the partial eclipse of the rotating stellar surface), we find the angle between the sky projections of the stellar spin axis and orbit normal to be λ = -1°.4 ± 1°.1. This is the third case of a "hot Jupiter" for which λ has been measured. In all three cases λ is small, ruling out random orientations with 99.96% confidence, and suggesting that the inward migration of hot Jupiters generally preserves spin-orbit alignment
We present measurements of the spin-orbit misalignments of the hot Jupiters HAT-P-41 b and WASP-79 b...
We present an improved measurement of the Rossiter-McLaughlin effect for the exoplanetary system HD ...
One possible diagnostic of planet formation, orbital migration, and tidal evolution is the angle ψ b...
We present spectroscopy of a transit of the exoplanet HD 189733b. By modeling the Rossiter-McLaughli...
We present high- precision radial velocity observations of HD 17156 during a transit of its eccentri...
Context. Several competing scenarios for planetary-system formation and evolution seek to explain ho...
Context. Several competing scenarios for planetary-system formation and evolution seek to explain ho...
Context. Several competing scenarios for planetary-system formation and evolution seek to explain ho...
Context. Several competing scenarios for planetary-system formation and evolution seek to explain ho...
International audienceContext. Several competing scenarios for planetary-system formation and evolut...
The short-period exoplanet HD 147506b (also known as HAT-P-2b) has an eccentric orbit, raising the p...
The discovery of giant planets orbiting <0.1AU of their host star was one of the most unexpected res...
We present new spectroscopic and photometric observations of the HAT-P-1 planetary system. Spectra o...
We have measured the alignment between the orbit of HATS-3b (a recently discovered, slightly inflate...
The Rossiter-McLaughlin (RM) effect is the distortion of stellar spectral lines that occurs during e...
We present measurements of the spin-orbit misalignments of the hot Jupiters HAT-P-41 b and WASP-79 b...
We present an improved measurement of the Rossiter-McLaughlin effect for the exoplanetary system HD ...
One possible diagnostic of planet formation, orbital migration, and tidal evolution is the angle ψ b...
We present spectroscopy of a transit of the exoplanet HD 189733b. By modeling the Rossiter-McLaughli...
We present high- precision radial velocity observations of HD 17156 during a transit of its eccentri...
Context. Several competing scenarios for planetary-system formation and evolution seek to explain ho...
Context. Several competing scenarios for planetary-system formation and evolution seek to explain ho...
Context. Several competing scenarios for planetary-system formation and evolution seek to explain ho...
Context. Several competing scenarios for planetary-system formation and evolution seek to explain ho...
International audienceContext. Several competing scenarios for planetary-system formation and evolut...
The short-period exoplanet HD 147506b (also known as HAT-P-2b) has an eccentric orbit, raising the p...
The discovery of giant planets orbiting <0.1AU of their host star was one of the most unexpected res...
We present new spectroscopic and photometric observations of the HAT-P-1 planetary system. Spectra o...
We have measured the alignment between the orbit of HATS-3b (a recently discovered, slightly inflate...
The Rossiter-McLaughlin (RM) effect is the distortion of stellar spectral lines that occurs during e...
We present measurements of the spin-orbit misalignments of the hot Jupiters HAT-P-41 b and WASP-79 b...
We present an improved measurement of the Rossiter-McLaughlin effect for the exoplanetary system HD ...
One possible diagnostic of planet formation, orbital migration, and tidal evolution is the angle ψ b...