+ 34 958 249061-62 fqm292@ugr.es

Stellar Evolution

Stellar Structure

Nucleosynthesis

Chemical Evolution of the Galaxies

Asteroseismology & Planet Detection

Infrared Astronomy from Antarctica

Thermonuclear explosions

AGB stars

About Us

We study the evolution of low and intermediate mass stars (M < 8 M): the mixing and nucleosynthesis processes occurring in their interiors, their surface chemical composition, final outcome as white dwarfs and/or thermonuclear supernovae, and their use in cosmology and the chemical evolution of the Universe, all both from the theoretical and observational points of view. We do also asteroseismology from space.