Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991acasn..32..389c&link_type=abstract
(Acta Astronomica Sinica, vol. 32, no. 4, 1991, p. 389-396) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 16, no. 2,
Astronomy and Astrophysics
Astronomy
Carbon Stars, M Stars, Silicates, Spectrum Analysis, Stellar Spectra, Absorption Spectra, Color-Color Diagram, Infrared Astronomy Satellite, Infrared Photometry, S Stars, Stellar Evolution, Stellar Spectrophotometry
Scientific paper
Twenty-three carbon stars with IRAS LRS 2n, 3n, and 6n are presented, of which seven samples have been identified to have 10 microns silicate features. It is determined that on the IRAS color-color diagram most of the samples are located in the M star region or in the overlapping region of S-type stars and carbon stars. Thus the circumstellar shells of the stars are either oxygen rich or are undergoing the stage of transition from the oxygen rich to the carbon rich.
Bao Meng-Xian
Chen Pei-Sheng
Gao Heng
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