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