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20062026
most citedGravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars

612 citations · 6.1k across the 85 of their papers we have counts for

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Showing 2010Show all

6 papers · 1 filter

astro-ph.SR2010★ 182 cited

The universal red-giant oscillation pattern; an automated determination with CoRoT data

B. Mosser, K. Belkacem, M. J. Goupil +12

The CoRoT and Kepler satellites have provided thousands of red-giant oscillation spectra. The analysis of these spectra requires efficient methods for identifying all eigenmode par…

astro-ph.SR2010★ 15 cited

Turbulent eddy-time-correlation in the solar convective zone

K. Belkacem, R. Samadi, M. J. Goupil +3

Theoretical modeling of the driving processes of solar-like oscillations is a powerful way of understanding the properties of the convective zones of solar-type stars. In this fram…

astro-ph.SR2010★ 9 cited

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

C. Karoff, W. J. Chaplin, T. Appourchaux +46

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 scien…

astro-ph.SR2010★ 236 cited

Red-giant seismic properties analyzed with CoRoT

B. Mosser, K. Belkacem, M. J. Goupil +10

The CoRoT 5-month long observation runs give us the opportunity to analyze a large variety of red-giant stars and to derive fundamental stellar parameters from their asteroseismic…

astro-ph.SR2010★ 241 cited

Solar-like oscillations in low-luminosity red giants: first results from Kepler

T. R. Bedding, D. Huber, D. Stello +47

We have measured solar-like oscillations in red giants using time-series photometry from the first 34 days of science operations of the Kepler Mission. The light curves, obtained w…

astro-ph.SR2010★ 154 cited

The asteroseismic potential of Kepler: first results for solar-type stars

W. J. Chaplin, T. Appourchaux, Y. Elsworth +105

We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5d of science operations, reveal hi…