Physics
Scientific paper
Jan 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986s%26w....25...23g&link_type=abstract
Sterne und Weltraum (ISSN 0039-1263), vol. 25, Jan. 1986, p. 23-25. In German.
Physics
Carbon Stars, Hertzsprung-Russell Diagram, Main Sequence Stars, Stellar Evolution, Doppler Effect, Stellar Spectra, Stellar Temperature
Scientific paper
The theoretical implications of the discovery of the carbon star G77 - 61 in the main sequence of the HR diagram are considered. The nature of carbon stars is reviewed, and methods for determining the characteristics of stars, and in particular those of G77 - 61, are discussed. The evolutionary status of the carbon star G77 - 61 is examined.
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