– Laboratory astrochemistry.  In collaboration with astronomers, we try to mimic processes that takes place in red-giant stars, supernovae or nebulae, using UHV technologies and surface science characterization techniques. This research line is framed on the NANOCOSMOS project

– Surface astrophysics and nanophotonics. Profiting from advanced surface science characterization techniques we model the interaction, reactivity, and luminescence of aromatic-aliphatic molecules on interstellar dust grains. 

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