RESEARCH AREAS
1
The Milky Way's Center:
Study of the inner regions of the galaxy, including the bulge and nuclear disk, to understand their early formation and evolution. This includes the analysis of complex structures, interstellar extinction, and the characterization of stellar and gas components.
2
The Solar Neighborhood:
Research on the chemical, kinematic, and evolutionary properties of stars near the Sun. It focuses on establishing precise calibration standards, essential for interpreting galactic and extragalactic data.
3
The Interstellar Medium (ISM):
Exploration of the physical properties of the interstellar gas and its relationship with star formation in different environments of the Milky Way. This includes the use of advanced observatories such as ALMA to map molecular clouds and assess star formation conditions.
4
The Interactions of the Milky Way:
Study of the galaxy's environment to understand how external interactions, such as accretion events, influence its evolution. This is complemented by high-resolution numerical simulations that model galactic formation processes and comparisons with other similar galaxies.
These lines of research combine observations, modeling, and data analysis to address fundamental questions about the structure, evolution, and dynamics of our galaxy, driving advancements in astrophysics both nationally and internationally.