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What is Carbon-Rich Dust in Magellanic Clouds about?

This document summarizes the results of analyzing infrared spectra of carbon-rich objects that have evolved past the asymptotic giant branch (AGB) phase in the Magellanic Clouds. The spectra reveal a variety of dust properties including fullerenes, polycyclic aromatic hydrocarbons (PAHs), aliphatic hydrocarbons, and several unidentified features. The analysis finds evidence for fullerenes in 3 new sources and questions previous identifications of fullerenes in 3 other sources. It confirms that strong 11 mic

Author

crocoali

Language

EN