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...
Towards the understanding of the late stages of stellar evolution and the formation of complex organic molecules
Most of the stars (M < 8 solar masses, Ms) end their lives with a phase of strong mass loss on the Asymptotic Giant Branch (AGB), just before they form...
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...
The Transiting Exoplanet Survey Satellite (TESS) is a NASA mission that started scientific operations in July 2018. Over two years it will cover the entire sky...
Unravelling the dark universe from the Canary Island observatories - UNDARK
Astrophysical and cosmological observations imply that only 5% of the energy of the Universe is made of conventional matter. The rest is composed by a new type...
UNVEILING THE COMPLEXITY OF RADIO FOREGROUNDS FOR THE DETECTABILITY OF THE CMB POLARIZATION B-MODE
The aim of RadioForegroundsPlus is to combine the nine Planck all-sky (30-857 GHz) maps, with three unique low-frequency data sets: the QUIJOTE maps (at 11, 13...
Unveiling the missing populations of X-ray binaries: dormant black holes and ultra-compact systems
X-ray binaries are excellent laboratories to study the physics of relativistic stars. On the one hand, they provide robust evidence for the existence of black...
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...