A semi-automatic procedure for abundance determination of A- and F-type stars
A variety of physical processes leading to different types of pulsations and chemical compositions are observed between A- and F-type stars. To investigate the underlying mechanisms responsible for these processes in stars with similar locations in the Hertzsprung-Russell diagram, an accurate abundance determination is needed, among others. Here
Hekker, S. et al.
Fecha de publicación:
7
2009