Evidence for hydrogenated amorphous carbon in the Red Rectangle

Details Evidence for hydrogenated amorphous carbon in the Red Rectangle Evidence for hydrogenated amorphous carbon in the Red Rectangle

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.215..259d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 215, July 15, 1985, p. 259-263. NSERC-supported researc

Astronomy and Astrophysics

Astronomy

76

Amorphous Materials, Astronomical Spectroscopy, Carbon, Cosmic Dust, Interstellar Matter, Nebulae, Absorption Spectra, Emission Spectra, Hydrogenation, Interstellar Extinction

Scientific paper

The absence of oxygen-rich dust in the Red Rectangle offers a unique
opportunity of observing the effects of one component of dust over a
wide spectral range. Observations and new laboratory data suggest that
the dust observed in the Red Rectangle is carbon-rich with a composition
similar to that of hydrogenated amorphous carbon (HAC).

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