192 citations · 292 across the 7 of their papers we have counts for
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Nonlinear seismic scaling relations
T. Kallinger, P. G. Beck, D. Stello +1
In recent years the global seismic scaling relations for the frequency of maximum power and for the large frequency separation have caught the attention of various fields of astrop…
Probing seismic solar analogues through observations with the NASA Kepler space telescope and HERMES high-resolution spectrograph
P. G. Beck, D. Salabert, R. A. García +21
Stars similar to the Sun, known as solar analogues, provide an excellent opportunity to study the preceding and following evolutionary phases of our host star. The unprecedented qu…
Magnetic activity of seismic solar analogs
D. Salabert, R. A. Garcia. P. G. Beck, the SSA team
We present our latest results on the solar-stellar connection by studying 18 solar analogs that we identified among the Kepler seismic sample (Salabert et al., 2016a). We measured…
Testing Asteroseismic Scaling Relations using Eclipsing Binaries in Star Clusters and the Field
K. Brogaard, J. Jessen-Hansen, R. Handberg +10
The accuracy of stellar masses and radii determined from asteroseismology is not known! We examine this issue for giant stars by comparing classical measurements of detached eclips…
Oscillating red-giant stars in eccentric binary systems
P. G. Beck, K. Hambleton, J. Vos +4
The unparalleled photometric data obtained by NASA's Kepler Space Telescope has led to improved understanding of red-giant stars and binary stars. We discuss the characterization o…
Kepler White Paper: Asteroseismology of Solar-Like Oscillators in a 2-Wheel Mission
W. J Chaplin, H. Kjeldsen, J. Christensen-Dalsgaard +53
We comment on the potential for continuing asteroseismology of solar-type and red-giant stars in a 2-wheel Kepler Mission. Our main conclusion is that by targeting stars in the ecl…
Mixed modes in red-giant stars observed with CoRoT
B. Mosser, C. Barban, J. Montalban +15
The CoRoT mission has provided thousands of red-giant light curves. The analysis of their solar-like oscillations allows us to characterize their stellar properties. Up to now, the…