ANR VAHIIAThe challenges of this project consist in simulating through laboratory experiments, the chemical evolution of interstellar ices, and grains to understand the evolution of the organic matter during the life cycle of interstellar grains. Currently, our team is developing two complementary approaches to study this evolution. First, we are investigating the chemical reactivity that can occur within analogs of pristine or cometary ices, by working on small size systems (two or three reactants). Second, we are investigating the characterization of refractory residues formed during photolysis and warming of ice analogs without any degradation using an orbitrap apparatus. We propose to develop a new approach, which consists in implementi...
More than 140 gas-phase molecules have been detected in the interstellar (IS) medium or in circumste...
This contribution presents an original analytical system for studying volatile organic compounds (VO...
Context. Thermal annealing of interstellar ices takes place in several stages of star formation. Kno...
International audienceThis contribution addresses the different approaches that are developed in our...
WOS:000340701500051International audienceThis contribution presents an original analytical system fo...
WOS:000317632700055International audienceWe have developed a new laboratory approach to investigate ...
International audienceWe have developed a new laboratory approach to investigate the evolution of in...
We have developed a new laboratory approach to investigate the evolution of interstellar i...
WOS:000342571200013International audienceWe use Very High Resolution Mass Spectrometry for analyses ...
Studying the chemical evolution of the interstellar medium (ISM) is critical for understanding chemi...
Interstellar ices are submitted to energetic processes (thermal, UV, and cosmic-ray radiations) prod...
International audienceUsing laboratory experiments, we investigate the role of photo and thermal deg...
More than 140 gas-phase molecules have been detected in the interstellar (IS) medium or in circumste...
This contribution presents an original analytical system for studying volatile organic compounds (VO...
Context. Thermal annealing of interstellar ices takes place in several stages of star formation. Kno...
International audienceThis contribution addresses the different approaches that are developed in our...
WOS:000340701500051International audienceThis contribution presents an original analytical system fo...
WOS:000317632700055International audienceWe have developed a new laboratory approach to investigate ...
International audienceWe have developed a new laboratory approach to investigate the evolution of in...
We have developed a new laboratory approach to investigate the evolution of interstellar i...
WOS:000342571200013International audienceWe use Very High Resolution Mass Spectrometry for analyses ...
Studying the chemical evolution of the interstellar medium (ISM) is critical for understanding chemi...
Interstellar ices are submitted to energetic processes (thermal, UV, and cosmic-ray radiations) prod...
International audienceUsing laboratory experiments, we investigate the role of photo and thermal deg...
More than 140 gas-phase molecules have been detected in the interstellar (IS) medium or in circumste...
This contribution presents an original analytical system for studying volatile organic compounds (VO...
Context. Thermal annealing of interstellar ices takes place in several stages of star formation. Kno...