Galaxy evolution strongly depends on the physics of the interstellar medium (ISM). The ISM is permeated by magnetic fields (B-fields), in which magnetic energy is in close equipartition with the thermal and kinetic energy. This physical condition makes the B-fields dynamically important at several stages of galaxy evolution, affecting gas flows in

Diseño, construcción y primera luz del EMO-1, un observatorio casero con estación meteorológica integrada, monitoreo permanente del cielo y colaboración científica. Youtube:https://youtube.com/live/0PFICuLjOAE?feature=share Zoom:https://rediris.zoom.us/j/92934299413ID de reunión: 929 3429 9413

Massive stars are chemical factories producing key elements, they are progenitors of supernovae, neutron stars and black holes, and they play a crucial role in the formation and evolution of galaxies. Given their prevalence in binary systems, at the end of their lives they may produce double-compact objects, which are potential gravitational-wave

A relevant fraction of massive stars are runaways, moving with a significant peculiar velocity with respect to their environment. Kicks from supernova explosions in binary systems or the dynamical ejection of stars from clusters can account for the runaway genesis. We have used Gaia DR3 data to study the velocity distribution of massive O and Be

In this talk I will present how the orbital motion of the Moon and artificial satellites can be used to find gravitational wave backgrounds in the microHz band. I will finish with the prospects of dedicated missions of relatively low coast and possible mould-breaking impact

TBD

At present, our understanding of the formation history of the MW is limited due to the complexity of observing the imprints of accretion events and of reproducing them in numerical simulations. Moreover, though being the only galaxy, in which the Galactic potential can be probed in detail, the distribution of mass in the MW, and hence of the dark

TBD

De parranda cantando Isas y Folías