Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...369..515r&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 369, March 10, 1991, p. 515-528.
Astronomy and Astrophysics
Astrophysics
30
B Stars, Early Stars, Photosphere, Stellar Spectra, Ultraviolet Spectra, Carbon, Line Spectra, Nitrogen, Silicon, Stellar Systems, Stellar Winds
Scientific paper
A set of criteria for the classification of G stars from UV spectra alone, using standards drawn form the optical region, is developed. About 100 stars having normal MK spectral types in the range B0-B8, III-V, have been classified. The UV spectral types are found to be very consistent with the optical MK types, implying that it is possible to do two-dimensional spectral classification in the UV without any knowledge of the optical spectrum.
Rountree Janet
Sonneborn George
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