about
A study of interstellar aldehydes and enols as tracers of a cosmic ray-driven nonequilibrium synthesis of complex organic molecules.Three milieux for interstellar chemistry: gas, dust, and ice.Separating para and ortho water.Graphene etching on SiC grains as a path to interstellar polycyclic aromatic hydrocarbons formation.Differential electron emission from polycyclic aromatic hydrocarbon molecules under fast ion impactRadiative cooling of C₇⁻.Free-electron laser induced processes in thin molecular ice.Separation and conversion dynamics of nuclear-spin isomers of gaseous methanolInverse internal conversion in C4(-) below the electron detachment threshold.Quantum tunneling observed without its characteristic large kinetic isotope effects.XUV excitation followed by ultrafast non-adiabatic relaxation in PAH molecules as a femto-astrochemistry experiment.Diamond-like-carbon nanoparticle production and agglomeration following UV multi-photon excitation of static naphthalene/helium gas mixtures.Astrochemistry of dust, ice and gas: introduction and overview.Uniform Supersonic Chemical Reactors: 30 Years of Astrochemical History and Future Challenges.Accurate structural and spectroscopic characterization of prebiotic molecules: The neutral and cationic acetyl cyanide and their related species.Concluding remarks: astrochemistry of dust, ice and gas.Internal conversion outcompetes autodetachment from resonances in the deprotonated tetracene anion continuum.Non-covalent interaction of benzene with methanol and diethyl ether solid surfaces.Structural features of the carbon-sulfur chemical bond: a semi-experimental perspective.Accurate spectroscopy of polycyclic aromatic compounds: from the rotational spectrum of fluoren-9-one in the millimeter wave region to its infrared spectrum.Atom tunnelling in the reaction NH3+ + H2 → NH4+ + H and its astrochemical relevance.Resonances of the anthracenyl anion probed by frequency-resolved photoelectron imaging of collision-induced dissociated anthracene carboxylic acid.Stability of carbonaceous dust analogues and glycine under UV irradiation and electron bombardment.Slow photoelectron velocity-map imaging spectroscopy of the C9H7 (indenyl) and C13H9 (fluorenyl) anions.Vibrational fine structure of C5 via anion slow photoelectron velocity-map imaging.Synthesis of complex organic molecules in simulated methane rich astrophysical ices.Signatures of a quantum diffusion limited hydrogen atom tunneling reaction.A laboratory heterodyne emission spectrometer at submillimeter wavelengths.XUV-induced reactions in benzene on sub-10 fs timescale: nonadiabatic relaxation and proton migration.Antagonistic functionalized nucleation and oxidative degradation in combustive formation of pyrene-based clusters mediated by triplet O and O2 : theoretical study.Ultraviolet photodissociation action spectroscopy of gas-phase protonated quinoline and isoquinoline cations.Electron induced chemistry: a new frontier in astrochemistry.Polycyclic aromatic hydrocarbons--catalysts for molecular hydrogen formation.Efficient diffusive mechanisms of O atoms at very low temperatures on surfaces of astrophysical interest.Astrochemistry of transition metals? The selected cases of [FeN](+), [FeNH](+) and [(CO)2FeN](+): pathways toward CH3NH2 and HNCO.Interactions of adsorbed CO₂ on water ice at low temperatures.Hydrogenation of PAH molecules through interaction with hydrogenated carbonaceous grains.Theoretical model of the interaction of glycine with hydrogenated amorphous carbon (HAC).An ion trap time-of-flight mass spectrometer with high mass resolution for cold trapped ion experiments.Impact of oxygen chemistry on model interstellar grain surfaces.
P2860
Q28829936-5F0D918A-B2FE-4BB4-9533-5D932884E1D8Q30457136-C1FEC122-8B69-472F-BFAC-4B680839A745Q30848081-62D9C3B9-AF89-4013-A020-96A10FE98E39Q33357610-ECA3BF84-620F-4910-A630-DB83B5FF0E1DQ33912000-5A291370-3FC2-4F64-B37F-FEF910277BB7Q35120456-D5982E24-3DEC-4F8D-86F0-8529F6FB25FCQ35319451-129EF264-824A-451C-84AC-FB7E55409F2EQ35543188-51B5A2E8-EA43-429A-8625-9032901A03FFQ35733904-1AF5B497-5295-4700-8D45-7F3238B8E62FQ35764440-CF2AB9F4-25CA-4270-8C8A-483CEA200A9BQ36018308-995F60F1-E515-4A53-B9AD-CC245937116EQ36078868-25B47F38-A2CD-4A49-85F5-8CC6943C8378Q38562984-BF2A8112-A24E-4FA4-B95A-E0C7848A76A7Q38671541-8B9D3CF4-7B28-4E87-BEA4-252F3801808AQ38942782-86AA2325-C59A-4C33-A49F-65883E9D7801Q39115731-3CA74EED-E753-447F-910B-C1AF0B78CBD4Q39284178-DDF5C461-43F2-474C-817C-25093CAE262BQ39602946-FFF58D8D-C54F-42CA-9E1D-1FD70B5E1989Q41232939-E3B5CFF9-E46D-4067-B49D-C48F9DB0541AQ41579108-04A2EBF2-B6F1-48C9-B7DE-827B3ABD6E51Q41832810-7C5B6D31-F2EF-4383-964F-A4E3537E747DQ42292801-229E3B3B-702F-4DDC-B0AE-B5FE081EFEE6Q42698117-FA817088-F7A2-44AA-950C-74E52B4E446FQ45135364-C04508F4-8DB4-49CF-80EC-0C17064E188FQ45944303-EB29D73C-15DB-4693-AC8B-2C47BD0F12EEQ46238856-F821E1C5-BFC5-4B58-A6AA-232480387B9DQ46247020-6D875BA3-53B7-4434-AF5B-C371524EF3E5Q46255490-EC27FC28-7C25-4F44-B3F5-49114322EE21Q46340471-076E3961-AD36-489C-BE3C-0C993EB3F3ABQ46708507-B91AFACD-0B1B-477D-A3E0-62FAC4811439Q46721528-7DAC508B-394B-46B2-AA71-31779FE85567Q46827206-6479BD50-0EB9-47CA-9C16-62AEF4CBFC1DQ46827210-59569F1F-7E7A-4036-8A2C-B0638D51983EQ46827213-09B3EAD7-2E12-4C83-8156-0DB53AFA6B3DQ46827818-1872C01A-1DEB-4F31-8F8B-745D2E9E31E6Q46875707-67D10B5A-DB27-465F-BA0A-4D367930A4F8Q46967970-840AEF18-D15D-4732-B535-D7B6A13F4A3FQ47607069-281697ED-32A1-4C53-8592-C9410CB992A1Q47758415-9CD4D7B1-C62C-42E9-BE90-ECB6A72B7559Q47866775-584FE022-9102-4BB6-864E-BFF44D25F669
P2860
description
im Juli 2013 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в липні 2013
@uk
name
The molecular universe
@en
The molecular universe
@nl
type
label
The molecular universe
@en
The molecular universe
@nl
prefLabel
The molecular universe
@en
The molecular universe
@nl
P2860
P1476
The molecular universe
@en
P2093
A. G. G. M. Tielens
P2860
P304
P356
10.1103/REVMODPHYS.85.1021
P577
2013-07-12T00:00:00Z