Seismic analysis of 7-month-long timeseries of solar-like stars

S. Mathur, T. L. Campante, R. Handberg, T. Appourchaux, R. A. García, G. Houdek, C. Karoff, KASC WG1

Abstract.
Since the launch of Kepler, a few solar-like oscillating stars (5) have been observed during ~7 months (Q0 to Q3). These stars have magnitudes in the range 10.5 to 12 and effective temperatures spanning from 5400 to 6000K according to the KIC. This is the first time that such continuous seismic time series are available, leading to a high resolution in the power spectrum. We will present the results obtained with the extraction of the global parameters of the p modes of these stars as well as the results from preliminary peak-bagging.

Third Kepler Asteroseismology Workshop: 'Kepler Asteroseismology in Action'
Aarhus, Denmark
June 2010

Type: Poster