Large interstellar molecules

Details Large interstellar molecules Large interstellar molecules

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986qjras..27..403d&link_type=abstract

Royal Astronomical Society, Quarterly Journal (ISSN 0035-8738), vol. 27, Sept. 1986, p. 403-412. NSERC-supported research.

Astronomy and Astrophysics

Astronomy

6

Interstellar Matter, Molecular Clouds, Absorption Spectra, Aromatic Compounds, Chemical Properties, Ionization Potentials, Size (Dimensions), Thermodynamic Properties

Scientific paper

The correlation between physical properties and molecule size is investigated using a model based on the addition of fused aromatic rings to the benezene molecule. The behavior of large molecules (greater than 50 atom) under interstellar conditions is examined. The thermal properties and photodecomposition and chemical stability of aromatic molecules and small carbon particles are analyzed. The relation between ionization potential and photoelectric emission, as the size of the molecule increases, is studied. The procedures, based on the Platt relation (1960), for predicting absorption wavelengths for positively charge aromatic ions are described.

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