Name: Marco A. Gómez-Muñoz

Title: Binarity effect in AGB and post-AGB evolution

Abstract: The principal objective of this project is to explore how the
binarity affects the evolution of low- and intermediate-mass stars, from
the Asymptotic giant branch (AGB) phase to the white dwarf (WD) cooling
phase. We took all photometric data, from the ultraviolet (UV) to the
near infrared (NIR), of the known central stars of Planetary Nebulae
(CSPNe) to analyze its spectral energy distribution (SED). For those
resulted in a binary system, via observing a double component on its
SED, an analysis of the morphology, chemical abundances, and galactic
distribution will be made. This will let us pose constraints on the
evolution of before-mentioned binary systems.