Shapes of Dust Features in Carbon-rich Sources

Details Shapes of Dust Features in Carbon-rich Sources Shapes of Dust Features in Carbon-rich Sources

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000esasp.456..323v&link_type=abstract

ISO beyond the peaks: The 2nd ISO workshop on analytical spectroscopy. Eds. A. Salama, M.F.Kessler, K. Leech & B. Schulz. ESA-SP

Computer Science

Scientific paper

We have analysed the shapes of the infrared features observed in a number of carbon-rich proto-planetary nebulae. Based upon ISO SWS data we derive template shapes for two of the UIR emission features, the 21 μm feature, and two sub-components of the 30 μm feature: a narrower peak at 26 μm and a broad feature which extends from 26 to 42 μm. For five sources we give the breakdown of infrared emission in these features.

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