Maria Tsantaki
CAUP

Abstract
Precise stellar parameters are important in understanding the formation and evolution not only for stars but for their planets as well. I will talk about the method of deriving stellar parameters for solar-type stars by measuring the iron lines. I will also present some results of the HARPS survey from Sousa 2008 & 2011 and their impact on planet surveys.

2012 April 02, 13:30

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