During the final stages of their lives, stars with masses between one and eight times the mass of the Sun evolve along the asymptotic giant branch (AGB). AGB stars expand and loss a major fraction of their mass through stellar winds. The low temperature and high density of AGB winds provide ideal conditions for the condensation of dust grains in their circumstellar envelopes. Gas and dust are expelled into the interstellar medium, becoming an essential component for the formation of new stars and planets. Therefore, studying the type of dust (solid state organic or inorganic components) and

Early-type galaxies (ETGs) were historically considered as ‘boring’ objects by astronomers. This galaxy category encompasses lenticular and elliptical galaxies, which were thought as morphologically featureless systems with no star formation and therefore of little interest. However, with the advent of powerful integral field spectrographs and deep photometric images, ETGs have demonstrated not to be such ‘boring’ systems, but complex galaxies with a variety of dynamical, photometric, and stellar population’s properties. In fact, a major question of current astrophysics is still to determine