Abstract
In this chapter, we present an investigation of spin-orbit angles for planetary system candidates reported by the Kepler space telescope. By combining the rotational period \(P_s\) inferred from the flux variation due to starspots and the projected rotational velocity \(V\sin I_s\) and stellar radius obtained by a high resolution spectroscopy, we attempt to estimate the inclination \(I_s\) of the stellar spin axis with respect to the line-of-sight. For transiting planetary systems, in which planetary orbits are edge-on seen from us, the stellar inclination \(I_s\) can be a useful indicator of a spin-orbit alignment/misalignment. We conducted spectroscopic observations with Subaru/HDS for about 15 KOI systems, whose lightcurves show periodic flux variations. After detailed analyses of their lightcurves and spectra, it turned out that some of them are binaries, or the flux variations are too coherent to be caused by starspots, and consequently we could constrain stellar inclinations \(I_s\) for eight systems. Among them, KOI-262 and 280 are in good agreement with \(I_s=90^\circ \) suggesting a spin-orbit alignment, while at least one system, KOI-261, shows a possible spin-orbit misalignment. The results for KOI-257, 269, 367, and 974 are ambiguous, and can be explained with either misalignments or moderate differential rotation.
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The other parameters such as the original Gaussian width and macroturbulence dispersion are fixed in the simulation.
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Hirano, T. (2014). Toward the Measurements of Spin-Orbit Relations for Small Planets . In: Measurements of Spin-Orbit Angles for Transiting Systems. Springer Theses. Springer, Tokyo. https://doi.org/10.1007/978-4-431-54586-6_5
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