The group's research involves the study of the final phases of stellar evolution and its associated nucleosynthesis from both an observational and theoretical viewpoint. In particular, the group studies the structure, evolution and nucleosynthesis of AGB stars and the physics of the explosion of white dwarfs as thermonuclear supernovae, together with its applications in cosmology. The above aspects are covered within the general framework of the chemical evolution of the Universe.

The main lines of research are as follows:

- Optical and infrared astronomy.

- Astroparticles.

- Chemical evolution of the universe.

- Chemical composition of cool stars.

- Thermonuclear supernovae and cosmology.

- Asteroseismology and exoplanets.

- Stellar evolution and nucleosynthesis.


Web page of the group.