Massive stars are those with more than ~8 solar masses, the limit above which stars may undergo a core collapse supernova (SN) explosion at the end of its life...
-
GrantThe Multiple Early Channels of EvolutioN of mAssive Stars
-
GrantThe structure and evolution of galaxies and their outskirts
We propose to study the evolution of galaxies through detailed analysis of observational data obtained with the most modern ground- and space-based telescopes...
-
GrantThe whole sun project: untangling the complex physical mechanisms behind our eruptive star and its twins: "Whole sun"
The Sun is a magnetically active star with violent eruptions that can hit Earth´s magnetosphere and cause important perturbations in our technology-dependent...
-
GrantThick discs, relics of the infancy of galaxies
Galaxy discs are made of two components, the thin and the thick disc. Thick discs contain up to 50% of the baryonic mass of a galaxy. Because their stars are...
-
GrantTracking active galactic nuclei feedback from parsec to kiloparsec scales
Active galactic nuclei (AGN) feedback is the effect that nuclear activity produces in the interstellar and circumgalactic medium (ISM and CGM) of galaxies...
-
GrantWeave: Cluster Surveys: A New Vision of the role of the environment in Galazy Evolution
The environment plays a key role in the formation and evolution of galaxies. Clusters of galaxies are the most massive and virialized structures known in the...
-
GrantX-ray binaries: accretion, ejection and masses
Accreting black-holes and neutron stars in X-ray binaries provide an ideal laboratory for exploring the physics of compact objects, yielding not only...
-
GrantBRIDGES - Ultracool dwarfs modeling: the bridge between planets and stars
BRIDGES main aim is the study of physical properties of the atmospheres ultracool dwarfs andexoplanets, modelling their spectra and comparison them with...