The objective of the Juan de la Cierva-formacion grants is to promote the hiring of people with a doctorate degree by research organizations in Spain for a period of two years in order to strengthen the skills acquired during a first stage of postdoctoral training in a different center from the one where they completed their PhD. The annual amount

The objective of the Juan de la Cierva-training grants is to promote the hiring of work by research organizations or centros i+D españoles other than those in which they carried out their pre-doctoral training. The aids whose annual amount is 26,300 euros, are used to co-finance the salary and the business contribution of Social Security of the

The objective of the Juan de la Cierva-training grants is to promote the hiring of work by research organizations or Spanish i+D centers other than those in which they carried out their pre-doctoral training. The aids whose annual amount is 26,300 euros, are used to co-finance the salary and the business contribution of Social Security of the

The aim of NanoSpace is to determine the abundance, formation mechanisms and astrochemical role of carbonaceous nanoparticles in space. Carbon is ubiquitous in space; from small carbon and hydrocarbon molecules to fullerenes and large but currently unidentified polycyclic aromatic hydrocarbons, carbonaceous dust particles and ultimately life. The

The Local Group (LG) offers us a chance to test the present scenario of galaxy formation in ways that are impossible elsewhere. It contains about 50 know galaxies, most of which are dwarfs so faint that they would not be detected beyond the LG. Hence, ourunderstanding of low-mass galaxy formation physics, strongly tied to models of galaxy feedback

This proposal seeks the scientific exploitation of the project on Dynamics of cool-core galaxy clusters, the mapping Cosmological Galaxy Clusters, and the galaxy cluster surveys of the EUCLID space mission in the coming years. The objectives of the project here presented are: 1) To investigate the nature of galaxy clusters with cool-cores, their