Massive stars are the cornerstone of the dynamic and chemical evolution of the cosmos, enriching it as they evolve with chemically processed material that is blown away from their surface by energetic winds and eruption processes. Despite their importance, their evolution from cradle to death as spectacular supernova explosions still poses many

The purpose of the grants is to train doctors by financing employment contracts, under the predoctoral contract modality, so that predoctoral research staff in training can carry out a doctoral thesis associated with a research project financed by the grants for R&D projects of the State Subprogram for Knowledge Generation within the framework of

This project MATRYOSHKA (Mass Assembly TRaced bY glObular clusterS, tHe Key to gAlaxy evolution) aims to address three key questions in astrophysics: (i) how do galaxies grow in size and mass; (ii) what is the dark matter content of these galaxies; and (iii) whether the current cosmological paradigm is compatible with this picture. We propose to

Accreting black holes and neutron stars in X-ray binaries (XRBs) provide an ideal laboratory for studying compact object physics as well as the physics of accretionthe most efficient mechanism of energy production known. This project (XB-LAB), building on prior initiatives (AYA2017-83216-P, PID2021- 124879NB-I00, and PID2020-120323GB-I00) led by

The aim of this project is to carry out research on the complex dynamics of plasma and magnetic field structures in different layers of the solar atmosphere, with emphasis on their connectivity and energy balance. The project relies on the creation of theoretical models, advanced numerical simulations, the analysis of state-of-the-art observations