Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26as...60..365m&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 60, June 1985, p. 365-372. Research supported by the Consigl
Astronomy and Astrophysics
Astrophysics
31
Spectral Energy Distribution, Stellar Models, Stellar Spectrophotometry, Stellar Temperature, Astronomical Catalogs, Diameters, O Stars, Stellar Atmospheres
Scientific paper
The effective temperatures and angular diameters of nonsupergiant O9-G8 stars are determined from visible spectrophotometry. The results, which refer to 302 stars included in the Breger Catalogue, are derived from the comparison between the observed flux distributions and the predictions of Kurucz's models (1979). The uncertainties to be expected in individual results are discussed; their sizes are of the order of 5 percent in effective temperature and 10 percent in angular diameter.
Malagnini Maria Lucia
Morossi Carlo
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