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Mount Wilson S-Index of 94 Aqr A and 94 Aqr B
Most previous efforts to calibrate how rotation and magnetic activity depend on stellar age and mass have relied on observations of clusters, where isochrones from stellar... -
Asymmetry of oscillations in 43 Kepler stars
Oscillation properties are usually measured by fitting symmetric Lorentzian profiles to the power spectra of Sun-like stars. However, the line profiles of solar oscillations... -
Acoustic modes of 11 delta Scuti stars
The main goal of this work is to date young open clusters using delta Sct stars. Seismic indices as the large separation and the frequency at maximum power can help to constrain... -
Seismic global parameters of 2103 KIC
The space-borne missions CoRoT and Kepler opened up a new opportunity for better understanding stellar evolution by probing stellar interiors with unrivalled high-precision... -
Inclinations for RGBs from Kepler asteroseismology
Measuring stellar inclinations is fundamental to understand planetary formation and dynamics as well as physical conditions during star formation. Oscillation spectra of red... -
Active red giants asteroseismic & rotation param.
Oscillating red-giant stars have provided a wealth of asteroseismic information regarding their interiors and evolutionary states, and access to their fundamental properties... -
4 p-mode pulsators arrival times
We investigate variations in the arrival time of coherent stellar pulsations due to the light travel time effect to test for the presence of sub-stellar companions. Those... -
Stellar pulsators in the eclipsing binaries
Eclipsing binaries (EBs) are unique targets for measuring precise stellar properties and can be used to constrain stellar evolution models. In particular, it is possible to... -
Buoyancy radius of {gamma} Dor stars
Helioseismology and asteroseismology of red giant stars have shown that distribution of angular momentum in stellar interiors, and the evolution of this distribution with time... -
New variables and 2 delta Scuti pulsations
Dome C in Antarctica is a promising site for photometric observations thanks to the continuous night during the Antarctic winter and favorable weather conditions. We developed... -
Rotation in RGBs from Kepler asteroseismology
Asteroseismology allows us to probe stellar interiors. In the case of red giant stars, conditions in the stellar interior are such as to allow for the existence of mixed modes,... -
Spectral significance for 15 delta Scuti
It is known that the observed distribution of frequencies in CoRoT and Kepler {delta} Scuti stars has no parallelism with any theoretical model. Pre-whitening is a widespread... -
61 main-sequence and subgiant oscillations
Solar-like oscillations have been observed by Kepler and CoRoT in several solar-type stars, thereby providing a way to probe the stars using asteroseismology We provide the mode...
