Emission features in IRAS LRS spectra of MS,'S and SC stars
Part of the Lecture Notes in Physics book series (LNP, volume 291)
Exploiting the Infrared
We observe a progression of emission features in the 8–11 μm region in MS, S and SC stars that parallels their increasing C:O ratio and s-process enhancements.
KeywordsEmission Feature Component Feature Carbon Star Star Emission Underlying Continuum
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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© Springer Verlag 1987