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