O. Benomar

On the uncertain nature of the core of α Cen A

High-quality astrometric, spectroscopic, interferometric and, importantly, asteroseismic observations are available for

Asteroseismology of Solar-Type Stars with K2: Detection of Oscillations in C1 Data

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Spin-Orbit Alignment of Exoplanet Systems: Ensemble Analysis Using Asteroseismology

Cen A, which is the closest binary star system to earth. Taking all these constraints into account, we study the internal structure of the star by means of theoretical modelling. Using the Aarhus STellar Evolution Code (ASTEC) and the tools of Computational Bayesian Statistics, in particular a Markov chain Monte Carlo algorithm, we perform statistical inferences for the physical characteristics of the star. We find that

A DISTANT MIRROR: SOLAR OSCILLATIONS OBSERVED on NEPTUNE by the KEPLER K 2 MISSION

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Asymmetry of Line Profiles of Stellar Oscillations Measured by Kepler for Ensembles of Solar-like Oscillators: Impact on Mode Frequencies and Dependence on Effective Temperature

Cen A has a probability of approximately 40% of having a convective core. This probability drops to few percents if one considers reduced rates for the

Asteroseismic detection of latitudinal differential rotation in 13 Sun-like stars

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Reliability of stellar inclination estimated from asteroseismology: analytical criteria, mock simulations and Kepler data analysis

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Time-Series Analysis of Broadband Photometry of Neptune from K2

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Seismic analysis of four solar-like stars observed during more than eight months by Kepler

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Fast rotating solar-like stars using asteroseismic datasets

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