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Experimental techniques Fretting corrosion Atomic and molecular collisions Spectroscopy Helium Astrochemistry Quantum Monte Carlo Atmospheric chemistry Planetary atmospheres IR spectroscopy Chemistry Classical H2 Excited states Reaction products Astrophysics - Solar and Stellar Astrophysics Contact resistance Quantum theory Stars evolution Radio lines ISM Astrophysics Tropospheric lifetimes Astrometry Spectral line shape Chemical physics Linewidths Nitrogen Molecular physics Line profiles Pressure broadening Molecular beams Cold collisions Line shape parameters Contact voltage Stars oscillations Kinetics Reaction dynamics Molecular Physics Molecular collisions Raman spectra Isomers CRESU MCTDH Methods numerical Molecular data Laboratory astrophysics Vibrational states Plasma plume Low temperature chemical kinetics Astrophysics - Astrophysics of Galaxies Quantum physics Collisions Molecular processes Atmospheres Planets and satellites composition Chemical kinetics Photolysis Reaction kinetics and dynamics Spectral element methods X-ray scattering He Optical frequency comb spectroscopy Atomic and molecular physics Cold and ultra-cold collisions ISM molecules Helium clusters Stars solar-type Physique moléculaire Optical lattice Nanoparticles Binaries spectroscopic Ab initio calculations Density functional calculations Radial velocities Quantum chemistry Methods data analysis ISM abundances Reaction kinetics Titan Chemical reactions Asteroseismology Methods analytical ISM clouds Astrophysique de laboratoire Surveys Combustion Soot Stars interiors Stars fundamental parameters Dusty plasmas Collisional broadening Infrared absorption Potential energy surfaces Vibronic couplings Acetylene Low temperatures SAXS Quantum dynamics Hydrogen Low temperature chemistry