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Davies, G R; Chaplin, W J; Farr, W M; Garcia, R A; Lund, M N; Mathis, S; Metcalfe, T S; Appourchaux, T; Basu, S; Benomar, O; Campante, T L; Ceillier, T; Elsworth, Y; Handberg, R; Salabert, D; Stello, D
Monthly notices of the Royal Astronomical Society, 01/2015, Letnik: 446, Številka: 3Journal Article
The solar analogues 16 Cyg A and B are excellent asteroseismic targets in the Kepler field of view and together with a red dwarf and a Jovian planet form an interesting system. For these more evolved Sun-like stars we cannot detect surface rotation with the current Kepler data but instead use the technique of asteroseimology to determine rotational properties of both 16 Cyg A and B. We find the rotation periods to be ... and ..., and the angles of inclination to be ... and ..., for A and B, respectively. Together with these results we use the published mass and age to suggest that, under the assumption of a solar-like rotation profile, 16 Cyg A could be used when calibrating gyrochronology relations. In addition, we discuss the known 16 Cyg B star-planet eccentricity and measured low obliquity which is consistent with Kozai cycling and tidal theory. (ProQuest: ... denotes formulae/symbols omitted.)
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