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Autor:
William D. Cochran, Roberto Sanchis-Ojeda, Christoffer Karoff, Rasmus Handberg, William J. Chaplin, Howard Isaacson, D. W. Latham, Mia S. Lundkvist, Mikkel N. Lund, Geoffrey W. Marcy, Dennis Stello, Hans Kjeldsen, T. S. Metcalfe, Sarbani Basu, Jørgen Christensen-Dalsgaard, Joshua N. Winn, Debra A. Fischer, Steven D. Kawaler, Ronald L. Gilliland, Saskia Hekker, Guy R. Davies, Tiago L. Campante, Daniel Huber, Thomas Barclay, Timothy R. Bedding, Y. P. Elsworth, Andrea Miglio, Lars A. Buchhave, Jack J. Lissauer
Publikováno v:
Chaplin, W J, Sanchis-Ojeda, R, Campante, T L, Handberg, R, Stello, D, Winn, J N, Basu, S, Christensen-Dalsgaard, J, Davies, G R, Metcalfe, T S, Buchhave, L A, Fischer, D A, Bedding, T R, Cochran, W D, Elsworth, Y, Gilliland, R L, Hekker, S, Huber, D, Isaacson, H, Karoff, C, Kawaler, S D, Kjeldsen, H, Latham, D W, Lund, M N, Lundkvist, M, Marcy, G W, Miglio, A, Barclay, T & Lissauer, J J 2013, ' Asteroseismic Determination of Obliquities of the Exoplanet Systems Kepler-50 and Kepler-65 ', Astrophysical Journal, vol. 766, pp. 101 . https://doi.org/10.1088/0004-637X/766/2/101
Astrophysical Journal, 766(2). IOP Publishing Ltd.
The Astrophysical Journal
arXiv
Astrophysical Journal, 766(2). IOP Publishing Ltd.
The Astrophysical Journal
arXiv
Results on the obliquity of exoplanet host stars -- the angle between the stellar spin axis and the planetary orbital axis -- provide important diagnostic information for theories describing planetary formation. Here we present the first application