Oral comunication
I. M. Brandão
Abstract
The solar type star KIC 10273246 (within KASC known as 'Mulder') is one of stars selected for a continuous monitoring by the Kepler satellite. With approximately 7 months of continuous observations, unprecedented for solar-type stars other than the Sun, accurate oscillation frequencies were derived for KIC 10273246. Combining these with fundamental parameters derived from ground-based spectra collected with the FIES spectrograph we performed a detailed modelling of the star.
In this talk, we present the results of such analysis.
4th KASC workshop: “From unprecedented data to revolutionary science”
Boulder, Colorado, U.S.A.
2011 July
