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G.C. Sloan (NASA Ames), I.R. Little-Marenin (Wellesley), S.D. Price (Phillips Lab.)
1998, AJ, 115, 809
Full article (PDF)We have developed a classification system for the infrared spectral emission from carbon stars, using a sample of 96 bright carbon-rich variables associated with the asymptotic giant branch. In addition to the stellar contribution, most spectra include the 11.2 µm emission feature from SiC and either a smooth cool continuum from amorphous carbon or a secondary emission feature at 9.0 µm. We have identified a carbon-rich dust sequence along which the amorphous carbon component grows while the 9.0 µm feature declines in strength. Along this spectral sequence, the fraction of Miras increases, as does the period of variability, the mass-loss rate, and the thickness of the circumstellar shell. Thus the carbon-rich dust sequence appears to be an evolutionary sequence. One class of spectra shows a particularly strong 9.0 µm feature, enhanced C/O ratio, and several other unusual properties that suggest a different sequence, perhaps related to J stars.
Downloadable figures and tables (in postscript format):
| Fig. 1 (30k) |
Fig. 2 (88k) |
Fig. 3 (52k) |
Fig. 4 (34k) |
Fig. 5 (36k) |
Fig. 6 (28k) |
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| Tab. 1 (15k) |
Tab. 2 (35k) |
Tab. 3 (15k) |
Tab. 4 (15k) |
Tab. 5 (13k) |
Tab. 6 (15k) |
Tab. 7 (17k) |
Table 2, the catalog of spectral classifications, is also available as an ASCII file (8k).
Last modified 27 May, 2008. © Gregory C. Sloan and others.