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- W1990658043 abstract "view Abstract Citations (46) References (23) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Quenched Carbonaceous Composite. III. Comparison to the 3.29 Micron Interstellar Emission Feature Sakata, A. ; Wada, S. ; Onaka, T. ; Tokunaga, A. T. Abstract Laboratory data are presented showing that oxidized f-QCC, after heating to 500 C, has a 3.29 micron absorption feature that matches precisely the wavelength of the 3.29 micron interstellar emission feature. In addition, the width of the f-QCC (filmy quenched carbonaceous composite) feature is close to that of the 3.29 micron emission feature observed in NGC 7027, Orion, and IRAS 21282 + 5050. Laboratory spectra of polycyclic aromatic hydrocarbons (PAHs) were also obtained, and comparison of the f-QCC and PAH absorption spectra to that of the 3.29 micron emission feature indicates that the f-QCC provides a much better match. It is thus suggested that f-QCC is representative of the class of material giving rise to the emission features in the interstellar medium. Publication: The Astrophysical Journal Pub Date: April 1990 DOI: 10.1086/168642 Bibcode: 1990ApJ...353..543S Keywords: Cyclic Hydrocarbons; Emission Spectra; Infrared Spectra; Interstellar Matter; Aromatic Compounds; Line Spectra; Spectrum Analysis; Astrophysics; INFRARED: SPECTRA; INTERSTELLAR: GRAINS; LINE IDENTIFICATIONS full text sources ADS | data products SIMBAD (6)" @default.
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- W1990658043 date "1990-04-01" @default.
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- W1990658043 title "Quenched carbonaceous composite. III - Comparison to the 3.29 micron interstellar emission feature" @default.
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