Abstract
Our de-reddened fluxes, together with the ultraviolet measurements of Thompson et al. (1978), have been compared with those of Kurucz’s (1979) model atmospheres to derive effective temperatures of some O emission, Be and Ae stars. With the measured monochromatic fluxes we determined their angular diameters and luminosities. It is found that the majority of the stars are cooler than the Zero-Age Main Sequence (ZAMS), suggesting that they are slightly more evolved than ZAMS stars.
The observations were made at the Observatoire de Haute Provence (France) and La Silla (E.S.O., Chile).
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© 1986 D. Reidel Publishing Company
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Woo, Jo. (1986). Effective Temperatures, Radii, and Luminosities of O Emission, Be and Ae Stars. In: Kitamura, M., Budding, E. (eds) Third Asian-Pacific Regional Meeting of the International Astronomical Union. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4630-9_13
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DOI: https://doi.org/10.1007/978-94-009-4630-9_13
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