Statistics – Computation
Scientific paper
Apr 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60..276s&link_type=abstract
(Astronomicheskii Zhurnal, vol. 60, Mar.-Apr. 1983, p. 276-283) Soviet Astronomy (ISSN 0038-5301), vol. 27, Mar.-Apr. 1983, p. 1
Statistics
Computation
B Stars, F Stars, Main Sequence Stars, Spectral Energy Distribution, Stellar Models, Stellar Temperature, Computational Grids, Stellar Color
Scientific paper
The values of effective temperatures for main sequence stars on the basis of their "colors" and with the help of models are obtained. It is shown that there are systematic deviations between these values and the scale of effective temperatures. Further analysis shows that the most probable reason for these systematic deviations are either errors in absolute calibration of standard stars or incorrectly constructed grids of models.
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