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

S. Mathur, T. L. Campante, R. Handberg, T. Appourchaux, R. 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
2010 June

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Faculdade de Ciências da Universidade de Lisboa Universidade do Porto Faculdade de Ciências e Tecnologia da Universidade de Coimbra
Fundação para a Ciência e a Tecnologia COMPETE 2020 PORTUGAL 2020 União Europeia