Abstract

Asteroseismology of solar and stellar models.- New results on standard solar models.- Low heavy-element photospheric abundance: a challenge for solar modeling.- Comparisons between stellar models and reliability of the theoretical models.- Modeling the solar irradiance background via numerical simulation.- Helioseismology as a diagnostic of the solar interior.- Prospects for asteroseismology.- How asteroseismology can constrain the global parameters of solar-like star models.- Asteroseismology and the degeneracy of model solutions for subgiant stars.- Determining stellar radii using large separations: an error analysis.- The red-giant CoRoT target HR?7349.- ??Cas: a new candidate ??Cephei star. Atmospheric characterization and variability analysis.- CoRoT 102931335: a candidate ? Dor in an eclipsing binary.- A complex asteroseismic study of the hybrid B-type pulsator ? Eridani.- Asteroseismic modelling of the solar-like star ? Hydri.- Spectroscopic mode identification of main-sequence non-radially pulsating stars.- The PMS ? Scuti star PDS2.- Investigating the semi-regular light variations of the bright M5 supergiant: ? Herculis.- CoRoT observations of the young open cluster Dolidze 25.- Pulsation period changes as a tool to identify pre-zero age horizontal branch stars.- Semiconvective mixing in low-mass stars.- Sensitivity of the sub-photospheric flow fields inferred from ring-diagram analysis to the change on the solar model.- Accurate and versatile equations of state for the Sun and Sun-like stars.- Application of SAHA-S EOS to solar modeling.- Dynamic screening in solar and stellar nuclear reactions.- Charged-particle induced thermonuclear reaction rates of 3He(3He,2p)4He, 3He(4He,?)7Be and 7Be(p,?)8B by using the exact tunneling probability.- Effects of new nuclear reaction rates on the solar neutrino fluxes.- The role of the equation of state in models of very low-mass stars.- Elemental diffusion and segregation processes in partially ionized solar plasma.- Emulating the OPAL equation of state.- The chemical composition of the Sun.- The chemical composition of solar-type stars in comparison with that of the Sun.- The solar, exoplanet and cosmological lithium problems.- Helium and metal diffusion in the Sun and in cluster stars.- Radiative accelerations, accumulation of iron and thermohaline convection inside stars.- Convection in stellar models.- Some properties of the kinetic energy flux and dissipation in turbulent stellar convection zones.- Overshooting and semiconvection: structural changes and asteroseismic signatures.- Stellar turbulence and mode physics.- Numerical simulations of the ?-mechanism with convection.- Stochastic excitation of gravity modes in massive main-sequence stars.- New insights on the interior of solar-like pulsators thanks to CoRoT: the case of HD 49385.- Smooth models of overshooting at the base of the solar convective zone.- The solar differential rotation: a historical view.- A semi-analytic approach to angular momentum transport in stellar radiative interiors.- Effect of stellar rotation on oscillation frequencies.- 2-D models of rapidly rotating stars.- 2D solar modeling.- The butterfly diagram internal structure.- The discontinuous nature of chromospheric-activity evolution.- Future instrumentation for solar physics: a double channel MOF imager on board ASI Space Mission ADAHELI.- A new opportunity from space: PLATO mission.- Planning magneto-optical filters for the study of magnetic oscillations of the Sun.- Synthetic stellar and SSP libraries as templates for Gaia simulations.- Differential photometry of ? Scuti stars at Maidanak observatory.- Unveiling stellar cores via their flattening.- Interpreting the solar cycle changes in p-mode velocity amplitudes as seen in Sun-as-a-star observations.- Nuclear reactions.

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