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• Introductory Lecture The growth of molecular complexity in the Universe;Chemistry and cosmology;Extragalactic chemistry of molecular gas: lessons from the local universe;Raman association of H2 in the early universe;Are gas-phase models of interstellar chemistry tenable? The case of methanol;Observations of chemical differentiation in clumpy molecular clouds;General Discussion;Meteorite nanoparticles as models for interstellar grains: Synthesis and preliminary characterisation;Laboratory investigations of the role of the grain surface in astrochemical models;The formation of interstellar molecules via reactions on dust grain surfaces;The temperature-dependence of rapid low temperature reactions: experiment, understanding and prediction;Crossed-beam studies on the dynamics of the C + C2H2 interstellar reaction leading to linear and cyclic C3H + H and C3 + H2;Dissociative recombination of protonated methanol;General Discussion;Photoprocesses in protoplanetary disks;Reaction dynamics of carbon-bearing radicals in circumstellar envelopes of carbon stars;Carbon molecules in space: from astrochemistry to astrobiology;Laboratory measurements of the recombination of PAH ions with electrons: implications for the PAH charge state in interstellar clouds;Structure of vapour deposited adenine on a nanostructured perovskite surface studied by STM;VUV spectroscopy and photo-processing of astrochemical ices: an experimental study;Comparative studies of O2 and N2 in pure, mixed and layered CO ices;General Discussion;New trends in cometary chemistry;Between heaven and Earth: the exploration of Titan;Hydrogen cyanide polymers, comets and the origin of life;Small-scale-structure of the interstellar medium probed through diffuse band observations;Polycyclic aromatic hydrocarbons, carbon nanoparticles and the diffuse interstellar bands;General Discussion;Concluding Remarks Future directions in astrochemistry

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• Introductory Lecture The growth of molecular complexity in the Universe;Chemistry and cosmology;Extragalactic chemistry of molecular gas: lessons from the local universe;Raman association of H2 in the early universe;Are gas-phase models of interstellar chemistry tenable? The case of methanol;Observations of chemical differentiation in clumpy molecular clouds;General Discussion;Meteorite nanoparticles as models for interstellar grains: Synthesis and preliminary characterisation;Laboratory investigations of the role of the grain surface in astrochemical models;The formation of interstellar molecules via reactions on dust grain surfaces;The temperature-dependence of rapid low temperature reactions: experiment, understanding and prediction;Crossed-beam studies on the dynamics of the C + C2H2 interstellar reaction leading to linear and cyclic C3H + H and C3 + H2;Dissociative recombination of protonated methanol;General Discussion;Photoprocesses in protoplanetary disks;Reaction dynamics of carbon-bearing radicals in circumstellar envelopes of carbon stars;Carbon molecules in space: from astrochemistry to astrobiology;Laboratory measurements of the recombination of PAH ions with electrons: implications for the PAH charge state in interstellar clouds;Structure of vapour deposited adenine on a nanostructured perovskite surface studied by STM;VUV spectroscopy and photo-processing of astrochemical ices: an experimental study;Comparative studies of O2 and N2 in pure, mixed and layered CO ices;General Discussion;New trends in cometary chemistry;Between heaven and Earth: the exploration of Titan;Hydrogen cyanide polymers, comets and the origin of life;Small-scale-structure of the interstellar medium probed through diffuse band observations;Polycyclic aromatic hydrocarbons, carbon nanoparticles and the diffuse interstellar bands;General Discussion;Concluding Remarks Future directions in astrochemistry

Select Guide Rating

• Introductory Lecture The growth of molecular complexity in the Universe;Chemistry and cosmology;Extragalactic chemistry of molecular gas: lessons from the local universe;Raman association of H2 in the early universe;Are gas-phase models of interstellar chemistry tenable? The case of methanol;Observations of chemical differentiation in clumpy molecular clouds;General Discussion;Meteorite nanoparticles as models for interstellar grains: Synthesis and preliminary characterisation;Laboratory investigations of the role of the grain surface in astrochemical models;The formation of interstellar molecules via reactions on dust grain surfaces;The temperature-dependence of rapid low temperature reactions: experiment, understanding and prediction;Crossed-beam studies on the dynamics of the C + C2H2 interstellar reaction leading to linear and cyclic C3H + H and C3 + H2;Dissociative recombination of protonated methanol;General Discussion;Photoprocesses in protoplanetary disks;Reaction dynamics of carbon-bearing radicals in circumstellar envelopes of carbon stars;Carbon molecules in space: from astrochemistry to astrobiology;Laboratory measurements of the recombination of PAH ions with electrons: implications for the PAH charge state in interstellar clouds;Structure of vapour deposited adenine on a nanostructured perovskite surface studied by STM;VUV spectroscopy and photo-processing of astrochemical ices: an experimental study;Comparative studies of O2 and N2 in pure, mixed and layered CO ices;General Discussion;New trends in cometary chemistry;Between heaven and Earth: the exploration of Titan;Hydrogen cyanide polymers, comets and the origin of life;Small-scale-structure of the interstellar medium probed through diffuse band observations;Polycyclic aromatic hydrocarbons, carbon nanoparticles and the diffuse interstellar bands;General Discussion;Concluding Remarks Future directions in astrochemistry