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2001ApJ...558L.129G - Astrophys. J., 558, L129-L132 (2001/September-2)
The far-infrared spectrum of hydrogenated amorphous carbon and the 21, 27, and 33 micron features in carbon-rich proto-planetary nebulae.
GRISHKO V.I., TERESZCHUK K., DULEY W.W. and BERNATH P.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Stars: Circumstellar Matter - Infrared: ISM - Infrared: Stars - ISM: Lines and Bands - ISM: Molecules - Stars: AGB and Post-AGB
Simbad objects: 2
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