Our main research topics focus on the study of massive stars and planetary systems.

Examples of massive stars include O, B, and A spectral-type supergiants, as well as Be-type stars. Studying the winds expelled by these stars reveals clues about their dynamics and chemical enrichment of the surrounding medium. Our studies are based on the use of hydrodynamic codes, analysis of spectra, and theoretical modeling.

A planetary system consists of objects orbiting a central star or stellar system. These objects can be planets, asteroids, comets, planetesimals, dust, among others. One of the objectives of studying these systems is to improve our understanding of their origin and evolution, diversity, and habitable zones. We study these systems through hydrodynamic and dynamic simulations, combined with theoretical modeling.

Research in Astrophysics is not limited to studying stars and planets in isolation. In our group, we seek synergies between these two areas. For example, exploring how massive stars influence the formation and evolution of planetary systems, thus obtaining a more comprehensive view of the phenomena under study.