Improved modeling of the Rossiter-McLAUGHLIN effect for transiting exoplanets

Astrophysical Journal

Volumn 742, Issue 2, 2011, Pages

  Hirano, Teruyuki ^a,b   Suto, Yasushi ^b,c,d   Winn, Joshua N ^a   Taruya, Atsushi ^b,c   Narita, Norio ^e   Albrecht, Simon ^a   Sato, Bun'Ei ^f  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^b UNIVERSITY OF TOKYO   (Japan)

^c UNIVERSITY OF TOKYO   (Japan)

^d PRINCETON UNIVERSITY   (United States)

^e NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^f TOKYO INSTITUTE OF TECHNOLOGY   (Japan)

Author keywords

planets and satellites: formation; planets and satellites: general; stars: rotation; techniques: radial velocities; techniques: spectroscopic

Indexed keywords

EID: 81255148002     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/742/2/69     Document Type: Article

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