THE STELLAR OBLIQUITY AND THE LONG-PERIOD PLANET IN THE HAT-P-17 EXOPLANETARY SYSTEM

THE STELLAR OBLIQUITY AND THE LONG-PERIOD PLANET IN THE HAT-P-17 EXOPLANETARY SYSTEM

We present the measured projected obliquity—the sky-projected angle between the stellar spin axis and orbital angular momentum—of the inner planet of the HAT-P-17 multi-planet system. We measure the sky-projected obliquity of the star to be $\lambda =19^{+14}_{-16}$ deg by modeling the Rossiter-McLa...

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Bibliografiska uppgifter
Huvudupphovsmän: Fulton, Benjamin J., Howard, Andrew W., Winn, Joshua Nathan, Albrecht, Simon H., Marcy, Geoffrey W., Crepp, Justin R., Bakos, Gaspar A., Johnson, John Asher, Hartman, Joel D., Isaacson, Howard, Knutson, Heather A., Zhao, Ming
Övriga upphovsmän: Massachusetts Institute of Technology. Department of Physics
Materialtyp: Artikel
Språk:en_US
Publicerad: Institute of Physics Publishing/American Astronomical Society 2014
Länkar:http://hdl.handle.net/1721.1/88625
https://orcid.org/0000-0002-4265-047X

Internet

http://hdl.handle.net/1721.1/88625
https://orcid.org/0000-0002-4265-047X

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