Diffusion Molecular processes Matched filters Millimeter wave devices Expansion 5 Abundances ISM Methods laboratory molecular Grain surface chemistry Molecules ISM Methods laboratory solid state Sea ice Indium gallium arsenide Amorphous water ice surface Interstellar medium Molecular data Individual objects L1521F Young stellar objects Galaxies clusters general Star formation Identification ISM Molecular clouds ISM individual objects L1544 Mixtures Modeling Identification -ISM Quantum tunneling Astrochemistry -radiative transfer -techniques Abundances -ISM Atomic processes Classification Deuteration Fourier transform infrared spectroscopy Circuits Laboratory Equilibrium temperatures Filtering 3 Circumstellar disks CRESU Rovibrational lines Astrochemistry – methods laboratory atomic – ISM atoms – ISM clouds – dust extinction – ISM molecules Interstellar medium ISM Astrophysics - Earth and Planetary Astrophysics Isomers 7 Interstellar molecules ISM jets and outflows Stars formation SMRT Molecular physics Interferometric -line Energy barriers Cosmological parameters Cold surfaces NO hydrogenation Reservoirs water Reactivity chemistry ISM kinematics and dynamics Graphite substrate Molecular hydrogen Protoplanetary disks Molecular Comets general ISM molecules Infrared spectroscopy IR RAIRS 1 Molecules Diodes ISM 6 ISM kinematic and dynamics Bandwidth Astrophysics - Astrophysics of Galaxies Astrochemistry -molecular processes -ISM Frequency CIMR Methods laboratory Nuclear spin isomer Oxygen Radiometer Radio lines ISM Stellar jets Astrophysics Isotopic exchange Protostars Scatterometer ISM atoms Molecules -methods 4 Astrochemistry Reactivity 2 Rotational temperature ISM clouds Astrochemistry line ASCAT Dust grains ISM abundances