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Shock waves Astrophysics Reaction products CRESUCHIRP Molecular physics Atmospheres Nanoparticles Surveys Atomic and molecular physics Low temperatures Astrophysics laboratory Reaction kinetics Chemical physics Quantum scattering Optical-optical double resonance spectroscopy Low temperature chemical kinetics Linewidths Collisions Potential energy Reaction kinetics and dynamics Catalogs Combustion Quantum Monte Carlo Spectrometers Binaries spectroscopic Line profiles Fretting corrosion X-ray scattering Microwave spectroscopy Contact voltage Quantum physics Stars fundamental parameters Atmospheric chemistry Planetary atmospheres Low temperature chemistry Cold collisions Line shape parameters Methods analytical Quantum dynamics Methods numerical Quantum theory Astrophysics - Astrophysics of Galaxies Molecular collisions Reaction dynamics Plasma plume Spectral element methods Astrochemistry MCTDH Contact resistance Proper motions Photolysis Methane Probes Collisional Potential energy surfaces Stimulated Raman spectroscopy Radial velocities Kinetics Atomic and molecular collisions Acetylene Pressure broadening Stars oscillations CRESU Molecular data Spectroscopy Stars formation Laboratory astrophysics Hydrogen Stars interiors Astrophysics - Solar and Stellar Astrophysics Nitrogen Vibronic couplings Optical frequency comb spectroscopy Cold and ultra-cold collisions Atomic and molecular collision Radio lines ISM Molecular processes ISM molecules Molecules Fourier transform infrared spectroscopy Tropospheric lifetimes ISM clouds ISM abundances Astrometry Asteroseismology Ab initio calculations Stars evolution Helium clusters Artificial Neuron Networks ANN Chemical kinetics Stars solar-type Spectral line shape Quantum chemistry Rate coefficients Soot Methods data analysis SAXS He Titan Collisional broadening