One of the main questions in Astrophysics is whether there are other Earths in the Galaxy. Our project is observational and technically prepared to address this question and lead to a significant progress on our understanding of the physical properties of planets, brown dwarfs, and stars, their formation mechanisms and evolution. We will conduct

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

Black holes (BHs) are the pinnacle of extreme gravity. They are responsible for the most violent phenomena observed in the Universe, from long gamma-ray bursts, tidal disruption events to gravitational waves (GW). Despite the recent growth in extragalactic BH discoveries by LIGO-VIRGO, our knowledge of the seed BH population is severely hindered by

ESTALLIDOS includes experts in observational astrophysics, numerical simulations, theoretical modeling, and instrumentation. Working together on "star formation" for more than 20 years, we have played a leading role in the development of the field (> 1000 papers, > 30 PhD Theses). Our strength lies in the complementarity among the different