Abstract
Most late-type giants and supergiants are losing mass in cool stellar winds. The only evidence for mass loss in single stars is the presence of a characteristic asymmetry deep in the core of photospheric lines. These asymmetries can be observed with modern high resolution coude echelle spectrographs and can be used for a study of mass loss rates and the wind structure in red giants. In this paper, we study the effects of partial redistribution functions RI-A and RII-A and complete redistribution on line profiles. The equation of transfer has been solved for a two level atom in the comoving frame.
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© 1985 D. Reidel Publishing company,Dordrecht, Holland
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Hempe, K. (1985). Partial Redistribution in the Winds of Red Giants. In: Beckman, J.E., Crivellari, L. (eds) Progress in Stellar Spectral Line Formation Theory. NATO ASI Series, vol 152. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5372-7_27
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DOI: https://doi.org/10.1007/978-94-009-5372-7_27
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