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- W2068278549 abstract "The JHKL' photometry and 2.3–4 μm spectrophotometry of some M giants, S type stars and carbon stars are presented in this paper. It is found that in combination with IRAS data, the energy spectra in 1–100 μm of S type stars are intermediate between those of M giants and carbon stars, which are obviously different. The spectrophotometry in the near infrared shows that, besides carbon stars, which have HCN and C2H2 strong absorptions at 3.1 μm, some S type stars have the similar but weaker absorption in the same spectral region. However, no trace of any absorption at 3.1 μm can be seen in M giants. These results probably provide more evidence for the M-S-C sequence in the late stage of stellar evolution." @default.
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- W2068278549 date "1992-10-01" @default.
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- W2068278549 title "1–100 μm energy spectra and 2.3–4 μm spectrophotometry of MSC stars" @default.
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- W2068278549 doi "https://doi.org/10.1016/0275-1062(92)90036-b" @default.
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