Institution: Ministerio de Ciencia, Innovación y Universidades
Acronym
MICIU
Grant
Thick 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...
Tracking 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...
Unveiling the Properties of Stellar Fosils in the Local Group Environment
The main objective of this project is the study of the primeval star formation in nearby systems. In particular, we will address this research in three...
VISION HOLISTICA DE LA EVOLUCION DE LA VIA LACTEA DEL PROGRAMA ATRAE EN EL MARCO DEL PROGRAMA ESTATAL PARA DESARROLLAR, ATRAER Y RETENER TALENTO DEL PLAN ESTATAL DE INVESTIGACIÓN CIENTÍFICA, TÉCNICA Y DE INNOVACIÓN 21-23
Within the general objective of enhancing the competitiveness of SECTI agents, this call specifically promotes the incorporation of consolidated talent in...
Weave: 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...
WEAVE: Exploring new scientific horizons through spectroscopic surveys.
The William Herschel Telescope (WHT) has been a key player in the take-off of Spanish astronomy in the last 25 years. With the access of the Spanish community...
X-ray binaries: accretion, ejection and dynamical masses
Black-holes and neutron stars are extremely important astrophysical objects, which become unique laboratories of extreme physics when found within X-ray...
X-ray binaries: accretion, ejection and dynamical masses
Black-holes and neutron stars are extremely important astrophysical objects, which become unique laboratories of extreme physics when found within X-ray...
Accreting black-holes and neutron stars in X-ray binaries provide an ideal laboratory for exploring the physics of compact objects, yielding not only...