Cosmic acceleration dominates the behavior of the recent universe, with some fundamentally new physics at its heart. Recent data gives a tantalizing suggestion that the dark energy behind it is more complicated than a cosmological constant.

Both observational and theoretical studies suggest that the magnetic field plays an important role in the process of massive star and cluster formation.

The Square Kilometre Array Observatory (SKAO) represents a monumental leap in radio astronomy technology, promising to redefine our understanding of the universe through its unprecedented capabilities.

The search for new worlds in the Galaxy in the past three decades has been highly successful and the prospects for the next decade are even brighter. A succession of space missions and ground-based facilities defines a timeline extending well into the 2030s.

Metals play a very important role in star formation and stellar evolution.

Unraveling the nature of dark matter (DM) stands as a primary objective in modern physics. I will present evidence suggesting deviations from the collisionless Cold DM (CDM) paradigm.

The inner solar system is populated by Interplanetary Dust Particles (IDPs) released from cometary trails and collisions between asteroids.

I will review the current status and future plans of the QUIJOTE (Q-U-I JOint TEnerife) experiment, a project with the aim of characterising the polarisation of the Cosmic Microwave Background, and other galactic or extragalactic physical processes that emit in microwaves in the frequency range 1

The talk will focus on two key areas. Part one will present the high-resolution imaging of Blazar TXS 2013+370, a study conducted as part of an M.Sc. thesis. This research aims to resolve the inner jet structure of the compact radio source TXS 2013+370 in total intensity and polarization.

En esta conferencia presentaremos, en primer lugar, una panorámica de la situación actual de la mujer en las STEM y en particular en la ingeniería, tratando de analizar qué factores pueden tener una mayor influencia en la situación actual.

I will present the Atacama Large Millimeter/submillimeter Array Band 7 observations at ~24 au spatial resolution of the CO (J=3-2) and H13CO molecular lines emission of the protostellar system HH 212 and compare them with the emission of the SiO (J=8-7) and SO (J=8-7) molecular lines.

Since we are children we have been taught what we are and we learn how to fit into a set of infinite boxes. Each of these boxes defines us and, at the same time, can be used to discriminate against us, in life and at work. Diversity exists and it could be an advantage for our society.

We apply horizontal visibility graphs (HVG) to study the complex network behavior for the delta Sct stars’ light curves observed by TESS. The delta Sct stars are pulsating stars with spectral types A0-F5 and intermediate masses between low-mass stars (≤ 1 Msun) and high-mass stars (≥ 2 Msun).