Asteroseismology of Solar-type Stars with Kepler I: Data Analysis

May, 2010
5 pages
Published in:
  • Astron.Nachr. 331 (2010) 972
e-Print:

Citations per year

201120122013402
Abstract: (arXiv)
We report on the first asteroseismic analysis of solar-type stars observed by Kepler. Observations of three G-type stars, made at one-minute cadence during the first 33.5d of science operations, reveal high signal-to-noise solar-like oscillation spectra in all three stars: About 20 modes of oscillation can clearly be distinguished in each star. We discuss the appearance of the oscillation spectra, including the presence of a possible signature of faculae, and the presence of mixed modes in one of the three stars.
Note:
  • 5 pages, 4 figure, submitted to Astronomische Nachrichten