Sources of the 13 micron feature associated with oxygen-rich circumstellar dust

G.C. Sloan (NASA Ames), P.D. LeVan (Phillips Lab./VTRP), I.R. Little-Marenin (Wellesley)

1996, ApJ, 463, 310

A search of the database of spectra from the IRAS Low-Resolution Spectrometer has revealed 13 µm emission features in 187 sources, most of which are associated with stars embedded within oxygen-rich circumstellar dust shells. Our sample is very incomplete, but we estimate that 40-50% of all sources with oxygen-rich dust on the asymptotic giant branch (AGB) exhibit emission features at 13 µm. The similarities of the galactic distribution, mean radial velocities, infrared colors, and other properties of the sample of 13 µm sources compared to the parent population of variables on the AGB suggest that the carrier of the 13 µm feature is commonly produced in oxygen-rich dust environments. A strikingly large fraction of SRb variables show 13 µm features, approximately 75-90%, suggesting that the formation and/or survival of the carrier of the 13 µm feature may be enhanced by the unusual pulsational properties of these variables.

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Last modified 27 May, 2008. © Gregory C. Sloan and others.