SIMBAD references

2015ApJ...801....3M - Astrophys. J., 801, 3 (2015/March-1)

Photometric amplitude distribution of stellar rotation of KOIs–Indication for spin-orbit alignment of cool stars and high obliquity for hot stars.

MAZEH T., PERETS H.B., McQUILLAN A. and GOLDSTEIN E.S.

Abstract (from CDS):

The observed amplitude of the rotational photometric modulation of a star with spots should depend on the inclination of its rotational axis relative to our line of sight. Therefore, the distribution of observed rotational amplitudes of a large sample of stars depends on the distribution of their projected axes of rotation. Thus, comparison of the stellar rotational amplitudes of the Kepler objects of interest (KOIs) with those of Kepler single stars can provide a measure to indirectly infer the properties of the spin-orbit obliquity of Kepler planets. We apply this technique to the large samples of 993 KOIs and 33,614 single Kepler stars in temperature range of 3500-6500 K. We find with high significance that the amplitudes of cool KOIs are larger, on the order of 10%, than those of the single stars. In contrast, the amplitudes of hot KOIs are systematically lower. After correcting for an observational bias, we estimate that the amplitudes of the hot KOIs are smaller than the single stars by about the same factor of 10%. The border line between the relatively larger and smaller amplitudes, relative to the amplitudes of the single stars, occurs at about 6000 K. Our results suggest that the cool stars have their planets aligned with their stellar rotation, while the planets around hot stars have large obliquities, consistent with the findings of Winn et al. and Albrecht et al. We show that the low obliquity of the planets around cool stars extends up to at least 50 days, a feature that is not expected in the framework of a model that assumes the low obliquity is due to planet-star tidal realignment.

Abstract Copyright:

Journal keyword(s): methods: observational - planets and satellites: dynamical evolution and stability - planet-star interactions - stars: rotation

VizieR on-line data: <Available at CDS (J/ApJ/801/3): table1.dat>

Simbad objects: 3357

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2015ApJ...801....3M and select 'bookmark this link' or equivalent in the popup menu


2021.05.06-09:52:40

© Université de Strasbourg/CNRS

    • Contact