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Astrophysique de laboratoire MCTDH Nitrogen Cold and ultra-cold collisions Hydroxyketones Linewidths ISM abundances CRESU Molecular Physics Low temperature chemical kinetics Atomic and molecular collisions Optical frequency comb spectroscopy Reaction kinetics and dynamics Optical lattice Atom-molecule reactions Helium Infrared absorption Vibrational states Arcs Experimental techniques Fretting corrosion Atomic and molecular physics Planets and satellites composition Collisional broadening Potential energy surfaces Raman spectra Binaries spectroscopic Acetylene Atom and radical reactions Reaction kinetics Argon Quantum physics Atmospheres Physique moléculaire Contact resistance Chemical kinetics Classical Collisions Vibronic couplings Tropospheric lifetimes Organic compounds Spectroscopy Soot Stars evolution Methods analytical Abundances Stars oscillations Chemical reactions Isomers Molecular processes Excited states Surveys Helium clusters Methods data analysis Radial velocities Low temperature chemistry Surface hopping Photolysis Quantum dynamics Quantum theory Kinetics Quantum Monte Carlo Dusty plasmas Astrochemistry Stars solar-type Molecular beams Molecular collisions Molecular physics Atmospheric chemistry Stars fundamental parameters Pressure broadening Astrophysics - Solar and Stellar Astrophysics Low temperatures Nanoparticles Astrophysics Chemical physics Planetary atmospheres ISM clouds Ab initio calculations Hydrogen Astrometry Plasma plume Reaction dynamics Contact voltage X-ray scattering Titan Stars interiors 4-hydroxy-4-methyl-2-pentanone Chemistry Laboratory astrophysics Spectral element methods Asteroseismology Radio lines ISM Automotive connectors Astrophysics - Astrophysics of Galaxies Molecular data Cold collisions SAXS ISM molecules Combustion