Abstract
The accuracy of the models of radiatively driven stellar winds can be checked by comparing predicted line profiles with the observed ones. A few years ago Martin Groenewegen and I have started a project to analyse the lineprofiles of UV wind lines of C III (λ 1175.66), C IV (A 1548.19 and 1550.76), N IV (A 1718.55), N V (A 1238.81 and 1242.80) and Si IV (A 1393.76 and 1402.77) observed in the high resolution spectra of 26 O-type stars and one B-supergiant. The observations are taken from the IUE atlas of Walborn et al. (1985).
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© 1991 Springer Science+Business Media Dordrecht
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Lamers, H.J.G.L.M. (1991). The Winds of O-Stars V: Tests of the Accuracy of the Radiation Driven Wind Models. In: Crivellari, L., Hubeny, I., Hummer, D.G. (eds) Stellar Atmospheres: Beyond Classical Models. NATO ASI Series, vol 341. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-3554-2_29
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