Seismic signatures of magnetic activity in solar-type stars observed by Kepler
arXiv:1806.04263 · doi:10.1017/S1743921318001229
Abstract
The properties of the acoustic modes are sensitive to magnetic activity. The unprecedented long-term Kepler photometry, thus, allows stellar magnetic cycles to be studied through asteroseismology. We search for signatures of magnetic cycles in the seismic data of Kepler solar-type stars. We find evidence for periodic variations in the acoustic properties of about half of the 87 analysed stars. In these proceedings, we highlight the results obtained for two such stars, namely KIC 8006161 and KIC 5184732.
arXiv comment4 pages, 1 figure, to appear in the Proceedings of the IAUS340
References in corpus (9)
- emcee: The MCMC Hammer
- Preparation of Kepler lightcurves for asteroseismic analyses
- Standing on the shoulders of Dwarfs: the asteroseismic LEGACY sample I - oscillation mode parameters
- CoRoT reveals a magnetic activity cycle in a Sun-like star
- Oscillation frequencies for 35 \Kepler solar-type planet-hosting stars using Bayesian techniques and machine learning
- Automated preparation of Kepler time series of planet hosts for asteroseismic analysis
- The influence of metallicity on stellar differential rotation and magnetic activity
- Signatures of magnetic activity in the seismic data of solar-type stars observed by Kepler
- Validation of solar-cycle changes in low-degree helioseismic parameters from the Birmingham Solar-Oscillations Network