TWO UPPER LIMITS ON THE ROSSITER-MCLAUGHLIN EFFECT, WITH DIFFERING IMPLICATIONS: WASP-1 HAS A HIGH OBLIQUITY AND WASP-2 IS INDETERMINATE

We present precise radial-velocity (RV) measurements of WASP-1 and WASP-2 throughout transits of their giant planets. Our goal was to detect the Rossiter-McLaughlin (RM) effect, the anomalous RV observed during eclipses of rotating stars, which can be used to study the obliquities of planet-hosting...

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Detalhes bibliográficos
Principais autores: Albrecht, Simon H., Winn, Joshua Nathan, Johnson, John Asher, Butler, R. Paul, Crane, Jeffrey D., Shectman, Stephen A., Thompson, Ian B., Narita, Norio, Sato, Bun'ei, Hirano, Teruyuki, Enya, Keigo, Fischer, Debra A.
Outros Autores: Massachusetts Institute of Technology. Department of Physics
Formato: Artigo
Idioma:en_US
Publicado em: Institute of Physics Publishing 2012
Acesso em linha:http://hdl.handle.net/1721.1/72323
https://orcid.org/0000-0002-4265-047X