Active galactic nuclei (AGN) feedback is the effect that nuclear activity produces in the interstellar and circumgalactic medium (ISM and CGM) of galaxies. Different modes of AGN feedback, which can be broadly divided into radiative/quasar and kinetic/radio, are now considered key processes in the evolution of massive galaxies by regulating black

Per the classical, textbook definition, planetary nebulae are the glowing shells of gas and dust expelled by single, Sun-like stars at the end of their lives as they evolve towards the white dwarf phase. However, there is growing evidence that a significant fraction, perhaps even a majority, of planetary nebulae are the result of binary

The Extremely Large Telescope (ELT), developed by the European Southern Observatory (ESO), will be the largest optical and infrared telescope ever built, with a 39-meter segmented mirror. This groundbreaking facility aims to transform our understanding of the Universe and offers significant opportunities for Spanish science and industry in advanced

We propose to study the evolution of galaxies through detailed analysis of observational data obtained with the most modern ground- and space-based telescopes. We will concentrate on two related important open questions in modern astrophysical research: how can deep imaging of large samples of galaxies uncover solutions to reported inconsistencies

AMS-02 (Alpha Magnetic Spectrometer) is a multi-purpose particle physics detector that was deployed in the International Space Station (ISS) on May 19, 2011. The experiment was designed to measure the flux of cosmic rays with unprecedented precision, which allows to study the origin and propagation of cosmic rays in the Milky Way. The main