Interstellar polycyclic aromatic hydrocarbons: the infrared emission bands, the excitation/emission mechanism, and the astrophysical implications.
about
State-of-the-art instruments for detecting extraterrestrial lifeThree milieux for interstellar chemistry: gas, dust, and ice.Infrared spectra of protonated polycyclic aromatic hydrocarbon molecules: azulene.Electron attachment on HI and DI in a uniform supersonic flow: thermalization of the electrons.Laser mass spectrometric detection of extraterrestrial aromatic molecules: mini-review and examination of pulsed heating effectsThe effect of the argon carrier gas in the multiphoton dissociation-ionization of tetracene.The inventory of interstellar materials available for the formation of the solar system.Charged polycyclic aromatic hydrocarbon clusters and the galactic extended red emission.An optical spectrum of a large isolated gas-phase PAH cation: C78H26(.)The Infrared Spectra of Polycyclic Aromatic Hydrocarbons with Excess Peripheral H Atoms (Hn-PAHs) and their Relation to the 3.4 and 6.9 µm PAH Emission Features.Mixed aliphatic and aromatic composition of evaporating very small grains in NGC 7023 revealed by the 3.4/3.3 μm ratio.Isomer-specific vibronic structure of the 9-, 1-, and 2-anthracenyl radicals via slow photoelectron velocity-map imaging.Irradiation of pyrimidine in pure H2O ice with high-energy ultraviolet photons.Radiolytic studies of naphthalene in the presence of water.Photosynthesis and photo-stability of nucleic acids in prebiotic extraterrestrial environments.A thermodynamic assessment of the potential synthesis of condensed hydrocarbons during cooling and dilution of volcanic gases.The synthesis of organic and inorganic compounds in evolved stars.Uniform Supersonic Chemical Reactors: 30 Years of Astrochemical History and Future Challenges.Formation of coronene:water complexes: FTIR study in argon matrices and theoretical characterisation.The interstellar chemistry of PAH cations.Laboratory photo-chemistry of PAHs: ionization versus fragmentationResonances of the anthracenyl anion probed by frequency-resolved photoelectron imaging of collision-induced dissociated anthracene carboxylic acid.Spectroscopy of prospective interstellar ions and radicals isolated in para-hydrogen matrices.A Free-Radical Pathway to Hydrogenated Phenanthrene in Molecular Clouds-Low Temperature Growth of Polycyclic Aromatic Hydrocarbons.Mechanism for the abiotic synthesis of uracil via UV-induced oxidation of pyrimidine in pure H(2)O ices under astrophysical conditions.Thermal desorption of C6H6 from surfaces of astrophysical relevance.The rotational spectra, electric dipole moments and molecular structures of anisole and benzaldehyde.Structural characterization of (C(2)H(2))(1-6) (+) cluster ions by vibrational predissociation spectroscopy.Thermal equation of state of solid naphthalene to 13 GPa and 773 K: in situ X-ray diffraction study and first principles calculations.Slow photoelectron velocity-map imaging spectroscopy of the C9H7 (indenyl) and C13H9 (fluorenyl) anions.The role of matrix material and CCl4 (electron acceptor) on the ionization mechanisms of matrix-isolated naphthalene.The anharmonic quartic force field infrared spectra of three polycyclic aromatic hydrocarbons: Naphthalene, anthracene, and tetracene.Electronic absorption spectroscopy of matrix-isolated polycyclic aromatic hydrocarbon cations. II. The phenanthrene cation (C14H10+) and its 1-methyl derivative.The anharmonic quartic force field infrared spectra of hydrogenated and methylated PAHs.Theoretical study of electronically excited radical cations of naphthalene and anthracene as archetypal models for astrophysical observations. Part I. Static aspects.Infrared spectra of ovalene (C32H14) and hydrogenated ovalene (C32H15˙) in solid para-hydrogen.Single photon infrared emission spectroscopy of the gas phase pyrene cation: support for a polycyclic aromatic hydrocarbon origin of the unidentified infrared emission bands.Bioastrophysical aspects of low energy ion irradiation of frozen anthracene containing water.The influence of coronene super-hydrogenation on the coronene-graphite interaction.Velocity-resolved [CII] emission and [CII]/FIR mapping along Orion with Herschel
P2860
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P2860
Interstellar polycyclic aromatic hydrocarbons: the infrared emission bands, the excitation/emission mechanism, and the astrophysical implications.
description
1989 nî lūn-bûn
@nan
1989 թուականի Դեկտեմբերին հրատարակուած գիտական յօդուած
@hyw
1989 թվականի դեկտեմբերին հրատարակված գիտական հոդված
@hy
1989年の論文
@ja
1989年論文
@yue
1989年論文
@zh-hant
1989年論文
@zh-hk
1989年論文
@zh-mo
1989年論文
@zh-tw
1989年论文
@wuu
name
Interstellar polycyclic aromat ...... he astrophysical implications.
@ast
Interstellar polycyclic aromat ...... he astrophysical implications.
@en
Interstellar polycyclic aromat ...... he astrophysical implications.
@nl
type
label
Interstellar polycyclic aromat ...... he astrophysical implications.
@ast
Interstellar polycyclic aromat ...... he astrophysical implications.
@en
Interstellar polycyclic aromat ...... he astrophysical implications.
@nl
prefLabel
Interstellar polycyclic aromat ...... he astrophysical implications.
@ast
Interstellar polycyclic aromat ...... he astrophysical implications.
@en
Interstellar polycyclic aromat ...... he astrophysical implications.
@nl
P2093
P356
P1476
Interstellar polycyclic aromat ...... he astrophysical implications.
@en
P2093
A G Tielens
J R Barker
L J Allamandola
P304
P356
10.1086/191396
P577
1989-12-01T00:00:00Z
P698
P819
1989ApJS...71..733A