<< back
Effective Temperatures of Solar-Type Stars

Joanna Molenda-Żakowicz
Astronomical Institute, University of Wroclaw

The effective temperatures, together with the surface gravities and the metallicities, are fundamental parameters for computing asteroseismic models. They need to be very precise and accurate now, in the era of the Kepler, in order to allow to compute dedicated asteroseismic models of stars. Unfortunately, it seems that deriving accurate effective temperature is by far more difficult to achieve than expected. In this talk, I discuss the difficulties related to determination of Teff, the external precision of our computations, and a few ideas how to approach those issues.

2012 December 13, 13:30

Centro de AstrofÝsica da Universidade do Porto (Auditorium)
Rua das Estrelas, 4150-762 Porto

Instituto de Astrof├şsica e Ci├¬ncias do Espa├žo Universidade do Porto Faculdade de Ciências da Universidade de Lisboa Funda├ž├úo para a Ci├¬ncia e a Tecnologia
Outreach at IA