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Water deuteration in star-forming regions : Contribution of Herschel/HIFI spe...
Water (H2O) is one of the most abundant molecules in the interstellar medium. In addition to being a primordial ingredient in the emergence of life, this species plays... -
Chemical and physical characterization of the first stages of protoplanetary ...
Low mass stars, like our Sun, are born from the collapse of a molecular cloud. The matter falls in the center of the cloud, creating a protoplanetary disk surrounding... -
High temperature kinetics and emission spectroscopy of hydrocarbons present i...
This work is devoted to the experimental investigation of the high temperature kinetics and spectroscopy of astrophysical gases. A versatile and existing High Enthalpy... -
Physical and chemical evolution of polycyclic aromatic hydrocarbons in photod...
Polycyclic aromatic hydrocarbons (PAHs) play a major role in the physics and chemistry of photodissociation regions (PDRs) in our galaxy. In these environments, the... -
Surface chemistry on interstellar grains in star-forming regions
The first stages of star formation are accompanied by an evolution of the chemistry, starting from simple molecules in cold dark clouds to the detection of complex... -
Experimental simulation of Titan's aerosols formation
This thesis studies the formation mechanisms and the composition of Titan's aerosols analogs, so called tholins. The study of the gas phase allowed identifying several... -
Physical and Chemical Conditions in the Horsehead Photodissociation Region
Molecular lines are used to trace the structure of the interstellar medium and the physical conditions of the gas in different environments, from high-z galaxies to...
