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