I present a discussion of the atomic input data required for state-of-the-art radiative acceleration calculations in magnetic stellar atmospheres, and of the numerical methods appropriate to this problem
Radiative accelerations are crucial quantities to study element diffusion in stars. They strongly de...
We compare four different methods to calculate radiative transfer through a magnetized stellar atmos...
Abstract. This and the following two chapters present a general intro-duction to the subject of obse...
International audienceWe present a revision of the results obtained by Alecian & Stift (\cite{als02}...
The influence of Zeeman splitting on radiative accelerations of chemical elements in stellar atmos...
International audienceAims.The present paper addresses some of the problems in the buildup of elemen...
The technique of model atmosphere calculation for magnetic Ap and Bp stars with polarized radiative ...
Aims. The present paper addresses some of the problems in the buildup of element stratification in s...
Element diffusion in the atmospheres of magnetic, chemically peculiar upper main sequence (CP) star...
Computations of polarization and intensity of radiation from a unit stellar surface area are present...
International audienceAccurate determination of radiative accelerations of the elements is critical ...
Atomic diffusion can have detectable effects in many kinds of stars, each time that mixing processes...
This and the following two chapters present a general introduction to the subject of observing magn...
Context: .We introduced the technique of model atmosphere calculation with polarized radiative trans...
Radiative accelerations are crucial quantities to study element diffusion in stars. They strongly de...
We compare four different methods to calculate radiative transfer through a magnetized stellar atmos...
Abstract. This and the following two chapters present a general intro-duction to the subject of obse...
International audienceWe present a revision of the results obtained by Alecian & Stift (\cite{als02}...
The influence of Zeeman splitting on radiative accelerations of chemical elements in stellar atmos...
International audienceAims.The present paper addresses some of the problems in the buildup of elemen...
The technique of model atmosphere calculation for magnetic Ap and Bp stars with polarized radiative ...
Aims. The present paper addresses some of the problems in the buildup of element stratification in s...
Element diffusion in the atmospheres of magnetic, chemically peculiar upper main sequence (CP) star...
Computations of polarization and intensity of radiation from a unit stellar surface area are present...
International audienceAccurate determination of radiative accelerations of the elements is critical ...
Atomic diffusion can have detectable effects in many kinds of stars, each time that mixing processes...
This and the following two chapters present a general introduction to the subject of observing magn...
Context: .We introduced the technique of model atmosphere calculation with polarized radiative trans...
Radiative accelerations are crucial quantities to study element diffusion in stars. They strongly de...
We compare four different methods to calculate radiative transfer through a magnetized stellar atmos...
Abstract. This and the following two chapters present a general intro-duction to the subject of obse...