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