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