Gerasim Khachatryan
CAUP

Abstract
In this seminar I will show the results derived with FUNDPAR program for 10 stars. We implemented a Fortran code that determines fundamental parameters of solar type stars from a list of Fe line equivalent widths.
The solution should verify three conditions in the standard method: ionization equilibrium, excitation equilibrium and independence between metallicity and equivalent widths.

2011 May 11, 13:30

IA/U.Porto
Centro de Astrofísica da Universidade do Porto (Classroom)
Rua das Estrelas, 4150-762 Porto