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