Galaxy evolution from the epoch of reionization to the nearby universe. Atomic and molecular gas in the interstellar medium of external galaxies, and relation to star formation and nuclear activity.

Magnetic fields in galaxies and in inter-and pre-galactic media. Spiral galaxies: warps, truncations, rotation curves. Theoretical models and observations.

Dense interstellar medium (interstellar dust and molecular gas) in external galaxies. Star formation in galaxies. Gaseous haloes of galaxies. Galaxies and their environment.

Galactic Evolution and Dynamics.

Star formation in nearby galaxies. Interstellar dust and gas. Interaction of stellar winds with the ISM. Stellar populations.

Formation and evolution of galaxies; observational study of abundances (and other properties) of HII regions by applying spectroscopic techniques.

Galaxy formation and evolution. The environment of galaxies and the large scale structure of the Universe. Stellar populations of galaxies. Dark matter haloes.

Spiral galaxies: kinematics and physical properties of the ionized interstellar medium (HII regions and diffuse ionized gas). Star formation. HII regions: physical, chemical and statistical properties.

Galaxy formation and evolution. Effects of the environment of galaxies. Star formation. Galaxy interactions. Astronomical data visualization.

Formation and evolution of low-mass galaxies in different environments. Chemical enrichment history and kinematics of galaxies.

Galaxy formation and evolution. Physical and chemical properties of star-forming galaxies and HII regions using spectroscopy. Galaxy interactions and environments. Supernova remnants.

Stellar populations in galaxies. Computation of star formation histories from spectroscopy (full-spectral fitting, nearby galaxies) and photometry (Colour-Magnitude Diagram fitting, Local Group galaxies and Milky Way). Halo dynamics and Milky Way accretion history (Gaia).

Cosmology. Large Scale Structures of the Universe. Galaxy formation and evolution. Galaxy interactions and environments. Machine Learning.

Galaxy formation and evolution. Influence of the local environment and large-scale structures. Atomic, molecular and ionized gas in galaxies. Development of tools for the analysis of galaxies surveys. Kinematics of galaxies.

Formation and evolution of galaxies. Role of the environment. Star formation in infrared, ultraviolet and visible. Relation between dust, gas and stars.