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