The unusual hydrocarbon emission from the early carbon star HD 100764: The connection between aromatics and aliphatics

G.C. Sloan (Cornell), M. Jura (UCLA), W.W. Duley (Waterloo), K.E. Kraemer (AFRL), J. Bernard-Salas (Cornell), W.J. Forrest (Rochester), B.A. Sargent (Rochester), A. Li (Missouri), D.J. Barry (Cornell), C.J. Bohac (Rochester), D.M. Watson (Rochester), J.R. Houck (Cornell).

2007, ApJ, 664, 1144

Full manuscript available from the ArXiv (0705.0905) or locally (PDF).

We have used the Infrared Spectrograph (IRS) on the Spitzer Space Telescope to obtain spectra of HD 100764, an apparently single carbon star with a circumstellar disk. The spectrum shows emission features from polycyclic aromatic hydrocarbons (PAHs) that are shifted to longer wavelengths than normally seen, as characteristic of “class C” systems in the classification scheme of Peeters et al. All seven of the known class C PAH sources are illuminated by radiation fields that are cooler than those which typically excite PAH emission features. The observed wavelength shifts are consistent with hydrocarbon mixtures containing both aromatic and aliphatic bonds. We propose that the class C PAH spectra are distinctive because the carbonaceous material has not been subjected to a strong ultraviolet radiation field, allowing relatively fragile aliphatic materials to survive.

Figures: Fig. 1 Fig. 2 Fig. 3 Fig. 4 Fig. 5 Fig. 6 Fig. 7

Home Library

Last modified 9 December, 2014. © Gregory C. Sloan and others.