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