The interpretation of the 3.2-3.5 micron emission feature in the spectrum of Comet P/Halley - Abundances in the comet and in interstellar matter

Details The interpretation of the 3.2-3.5 micron emission feature in the spectrum of Comet P/Halley - Abundances in the comet and in interstellar matter The interpretation of the 3.2-3.5 micron emission feature in the spectrum of Comet P/Halley - Abundances in the comet and in interstellar matter

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...207..162e&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 207, no. 1, Dec. 1988, p. 162-173.

Astronomy and Astrophysics

Astrophysics

29

Abundance, Emission Spectra, Halley'S Comet, Infrared Spectra, Interstellar Matter, Molecular Clouds, Molecular Spectra, Resonance Fluorescence, Solar Radiation

Scientific paper

The purpose of this paper is to try to analyze the various mechanisms and the nature of the possible emitters which can be responsible for the 3 μm cometary emission, in order to derive in each case, the amount of carbon required to account for the observed emission. As a second objective, the authors use these results, together will the relative abundances of parent molecules, to derive the relative elemental abundances of H, C, N and O in comet Halley, and try to compare these numbers with the abundances derived for interstellar dust.

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