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Abundances Astrochemistry Methods data analysis Collisions Stars oscillations Low temperatures Titan Arcs Helium Experimental techniques Raman spectra Argon Planets and satellites composition 4-hydroxy-4-methyl-2-pentanone Fretting corrosion Vibronic couplings Molecular data Nanoparticles Astrophysics - Solar and Stellar Astrophysics Atomic and molecular collisions Photolysis Linewidths Reaction kinetics and dynamics Physique moléculaire Chemical reactions Atmospheric chemistry Contact resistance Organic compounds Stars evolution Infrared absorption Binaries spectroscopic Soot Acetylene Hydrogen Quantum dynamics MCTDH Atomic and molecular physics Stars solar-type Quantum physics Dusty plasmas Stars interiors Combustion Spectroscopy ISM clouds Quantum Monte Carlo X-ray scattering Classical Astrometry Hydroxyketones Quantum theory Collisional broadening Molecular processes Ab initio calculations Radial velocities SAXS Chemical physics Laboratory astrophysics Nitrogen Cold collisions Surface hopping Contact voltage Chemical kinetics Methods analytical Molecular beams ISM molecules Density functional calculations Pressure broadening Optical frequency comb spectroscopy Astrophysique de laboratoire Vibrational states Atmospheres Kinetics ISM abundances Chemistry Molecular Physics Molecular collisions Reaction kinetics Optical lattice Astrophysics Helium clusters Low temperature chemical kinetics CRESU Low temperature chemistry Surveys Reaction dynamics Isomers Potential energy surfaces Planetary atmospheres Plasma plume Cold and ultra-cold collisions Molecular physics Spectral element methods Asteroseismology Excited states Astrophysics - Astrophysics of Galaxies Tropospheric lifetimes Stars fundamental parameters Atom and radical reactions Radio lines ISM IR spectroscopy