Luminescence from interstellar carbons - Evidence for diamond-like dust from extended red and near-infrared emission

Details Luminescence from interstellar carbons - Evidence for diamond-like dust from extended red and near-infrared emission Luminescence from interstellar carbons - Evidence for diamond-like dust from extended red and near-infrared emission

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.230p...1d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 230, Feb. 1, 1988, p. 1p-4p. NSERC-SERC-supported resea

Astronomy and Astrophysics

Astronomy

41

Carbon, Cosmic Dust, Diamonds, Interstellar Matter, Near Infrared Radiation

Scientific paper

Laboratory data on visible and near-infrared emission from hydrogenated amorphous carbon are correlated with observational data on extended red emission and near-infrared continua in astronomical objects. It appears that the observation of extended red emission is indicative of the presence of newly formed carbon dust that is rich in diamond-like material. The relationship between this material and normal interstellar dust is discussed.

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