Mélanie Godart

TL;DR: In this article, the authors investigated under what physical circumstances non-radial modes could be observable in red giants; what would be their amplitudes, lifetimes and heights in the power spectrum (PS).

TL;DR: CLES as mentioned in this paper is an evolution code recently developed to produce stellar models meeting the specific requirements of studies in asteroseismology, it offers the users a lot of choices in the input physics they want in their models and its versatility allows them to tailor the code to their needs and implement easily new features.

TL;DR: In this article, a physical explanation for the occurrence of macroturbulence in the atmospheres of hot massive stars, a phenomenon found in observations for more than a decade but that remains unexplained, is presented.

TL;DR: The Liège Oscillation code can be used as a stand-alone program or as a library of subroutines that the user calls from a Fortran main program of his own to compute radial and nonradial adiabatic oscillations of stellar models.

TL;DR: In this article, the authors used high-resolution spectra of 430 stars with spectral types in the range O4 - B9 (all luminosity classes) compiled in the framework of the IACOB project to provide new empirical clues about macroturbulent spectral line broadening in O- and B-type stars.