Microdiamonds and the 3.4 micrometer feature in protostellar sources

Details Microdiamonds and the 3.4 micrometer feature in protostellar sources Microdiamonds and the 3.4 micrometer feature in protostellar sources

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.207..309h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 207, no. 2, p. 309-311

Astronomy and Astrophysics

Astronomy

1

Absorption Spectra, Carbonaceous Chondrites, Diamonds, Infrared Astronomy, Interstellar Matter, Meteoritic Composition, Molecular Clouds, Protostars, Astronomical Spectroscopy, Chemical Composition, Ice, Optical Thickness, Stellar Spectra, Supernovae

Scientific paper

The optical constants of impure meteoritic microdiamonds are used to
calculate the 3.4 micrometers absorption profile of nanometer-sized
microdiamonds, and microdiamonds with water-ice coatings. It is shown
that the 3.4 micrometers feature observed in protostellar sources cannot
be easily explained on the basis of such models.

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