Two upper limits on the Rossiter-MCLAUGHLIN effect, with differing implications: WASP-1 has a high obliquity and WASP-2 is indeterminate

Astrophysical Journal

Volumn 738, Issue 1, 2011, Pages

  Albrecht, Simon ^a   Winn, Joshua N ^a   Johnson, John Asher ^b   Paul Butler, R ^c   Crane, Jeffrey D ^d   Shectman, Stephen A ^d   Thompson, Ian B ^d   Narita, Norio ^e   Sato, Bun'Ei ^f   Hirano, Teruyuki ^a,g   Enya, Keigo ^h   Fischer, Debra ⁱ  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c GEOPHYSICAL LABORATORY   (United States)

^d CARNEGIE OBSERVATORIES   (United States)

^e NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^f TOKYO INSTITUTE OF TECHNOLOGY   (Japan)

^g UNIVERSITY OF TOKYO   (Japan)

^h JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

ⁱ YALE UNIVERSITY   (United States)

Author keywords

planet star interactions; planetary systems; planets and satellites: formation; stars: rotation; techniques: spectroscopic

Indexed keywords

EID: 80052718070     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/738/1/50     Document Type: Article

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