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Polycyclic Aromatic Hydrocarbons Orbiting HD 233517, an Evolved Oxygen-Rich Red Giant

M. Jura·J. Bohac·B. Sargent·W. J. Forrest·J. Green·D. M. Watson·G. C. Sloan·F. Markwick-Kemper·C. H. Chen·J. Najita
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Abstract

We report spectra obtained with the Spitzer Space Telescope in the 5 to 35 micron range of HD 233517, an evolved K2 III giant with circumstellar dust. At wavelengths longer than 13 microns, the flux is a smooth continuum that varies approximately as frequency to the -5/3 power. For wavelengths shorter than 13 microns, although the star is oxygen-rich, PAH features produced by carbon-rich species at 6.3 microns, 8.2 microns, 11.3 microns and 12.7 microns are detected along with likely broad silicate emission near 20 microns. These results can be explained if there is a passive, flared disk orbiting HD 233517. Our data support the hypothesis that organic molecules in orbiting disks may be synthesized in situ as well as being incorporated from the interstellar medium.

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M. Jura, J. Bohac, B. Sargent, W. J. Forrest, J. Green, D. M. Watson, G. C. Sloan, F. Markwick-Kemper, C. H. Chen, J. Najita. 2005-12-14. Polycyclic Aromatic Hydrocarbons Orbiting HD 233517, an Evolved Oxygen-Rich Red Giant. https://doi.org/10.1086/500429

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