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Partial Redistribution in the Winds of Red Giants

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Part of the book series: NATO ASI Series ((ASIC,volume 152))

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

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-8870-1

  • Online ISBN: 978-94-009-5372-7

  • eBook Packages: Springer Book Archive

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