Add to ORKGWe provide evidence that the obliquities of stars with close-in giant planets were initially nearly random, and that the low obliquities that are often observed are a consequence of star-planet tidal interactions. The evidence is based on 14 new measurements of the Rossiter-McLaughlin effect (for the systems HAT-P-6, HAT-P-7, HAT
There are now more than 30 stars with transiting planets for which the stellar obliquity—or more pre...
We show that stars with transiting planets for which the stellar obliquity is large are preferential...
We have detected the Rossiter–Mclaughlin effect during a transit of WASP-47b, the only known hot Jup...
We provide evidence that the obliquities of stars with close-in giant planets were initially nearly ...
We provide evidence that the obliquities of stars with close-in giant planets were initially nearly ...
We measure the sky-projected stellar obliquities (λ) in the multiple-transiting planetary systems KO...
We investigate tidal dissipation of obliquity in hot Jupiters. Assuming an initial random orientatio...
We investigate tidal dissipation of obliquity in hot Jupiters. Assuming an initial random orientatio...
Hot Jupiters are intriguing because of their close proximity to the host star. Current theories have...
We measure a tilt of 86 ± 6 ◦ between the sky projections of the rotation axis of the WASP-7 star, a...
We measure the sky-projected stellar obliquities (λ) in the multiple-transiting planetary systems KO...
We measure the sky-projected stellar obliquities (λ) in the multiple-transiting planetary systems KO...
Two formation scenarios have been proposed to explain the tight orbits of hot Jupiters. They could b...
Measuring the obliquity distribution of stars hosting warm Jupiters may help us to understand the fo...
We show that stars with transiting planets for which the stellar obliquity is large are preferential...
There are now more than 30 stars with transiting planets for which the stellar obliquity—or more pre...
We show that stars with transiting planets for which the stellar obliquity is large are preferential...
We have detected the Rossiter–Mclaughlin effect during a transit of WASP-47b, the only known hot Jup...
We provide evidence that the obliquities of stars with close-in giant planets were initially nearly ...
We provide evidence that the obliquities of stars with close-in giant planets were initially nearly ...
We measure the sky-projected stellar obliquities (λ) in the multiple-transiting planetary systems KO...
We investigate tidal dissipation of obliquity in hot Jupiters. Assuming an initial random orientatio...
We investigate tidal dissipation of obliquity in hot Jupiters. Assuming an initial random orientatio...
Hot Jupiters are intriguing because of their close proximity to the host star. Current theories have...
We measure a tilt of 86 ± 6 ◦ between the sky projections of the rotation axis of the WASP-7 star, a...
We measure the sky-projected stellar obliquities (λ) in the multiple-transiting planetary systems KO...
We measure the sky-projected stellar obliquities (λ) in the multiple-transiting planetary systems KO...
Two formation scenarios have been proposed to explain the tight orbits of hot Jupiters. They could b...
Measuring the obliquity distribution of stars hosting warm Jupiters may help us to understand the fo...
We show that stars with transiting planets for which the stellar obliquity is large are preferential...
There are now more than 30 stars with transiting planets for which the stellar obliquity—or more pre...
We show that stars with transiting planets for which the stellar obliquity is large are preferential...
We have detected the Rossiter–Mclaughlin effect during a transit of WASP-47b, the only known hot Jup...