TY - JOUR
T1 - Asteroseismic Determination of the Stellar Rotation Period of the Kepler Transiting Planetary Systems and its Implications for the Spin-Orbit Architecture
AU - Suto, Yasushi
AU - Kamiaka, Shoya
AU - Benomar, Othman
N1 - Publisher Copyright:
© 2019. The American Astronomical Society. All rights reserved.
PY - 2019/5
Y1 - 2019/5
N2 - We measure the rotation periods of 19 stars in the Kepler transiting planetary systems, P rot,astero from asteroseismology and P rot,phot from the photometric variation of their light curves. Two stars exhibit two clear peaks in the Lomb-Scargle periodogram, neither of which agrees with the seismic rotation period. Other four systems do not show any clear peak, whose stellar rotation period is impossible to estimate reliably from the photometric variation; their stellar equators may be significantly inclined with respect to the planetary orbital plane. For the remaining 13 systems, P rot,astero and agree within 30%. Interestingly, 3 out of the 13 systems are in the spin-orbit resonant state in which with P orb,b being the orbital period of the innermost planet of each system. The corresponding chance probability is (0.2-4.7)% based on the photometric rotation period data for 464 Kepler transiting planetary systems. While further analysis of stars with reliable rotation periods is required to examine the statistical significance, the spin-orbit resonance between the star and planets, if confirmed, has important implications for the star-planet tidal interaction, in addition to the origin of the spin-orbit (mis-)alignment of transiting planetary systems.
AB - We measure the rotation periods of 19 stars in the Kepler transiting planetary systems, P rot,astero from asteroseismology and P rot,phot from the photometric variation of their light curves. Two stars exhibit two clear peaks in the Lomb-Scargle periodogram, neither of which agrees with the seismic rotation period. Other four systems do not show any clear peak, whose stellar rotation period is impossible to estimate reliably from the photometric variation; their stellar equators may be significantly inclined with respect to the planetary orbital plane. For the remaining 13 systems, P rot,astero and agree within 30%. Interestingly, 3 out of the 13 systems are in the spin-orbit resonant state in which with P orb,b being the orbital period of the innermost planet of each system. The corresponding chance probability is (0.2-4.7)% based on the photometric rotation period data for 464 Kepler transiting planetary systems. While further analysis of stars with reliable rotation periods is required to examine the statistical significance, the spin-orbit resonance between the star and planets, if confirmed, has important implications for the star-planet tidal interaction, in addition to the origin of the spin-orbit (mis-)alignment of transiting planetary systems.
KW - asteroseismology
KW - methods: data analysis
KW - planetary systems
KW - stars: rotation
KW - techniques: photometric
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U2 - 10.3847/1538-3881/ab0f33
DO - 10.3847/1538-3881/ab0f33
M3 - Article
AN - SCOPUS:85067339285
SN - 0004-6256
VL - 157
JO - Astronomical Journal
JF - Astronomical Journal
IS - 5
M1 - 172
ER -