Abstract
We study the relation between photospheric and wind parameters of LBV′s on the basis of self-consistent atmospheric models. Our theoretical model consists of a spherically extended, dynamical NLTE atmosphere for the radiative transfer and a modified CAK code for the hydrodynamics. These codes are combined in an iterative scheme to achieve self-consistency.
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References
Appenzeller, I. (1986) in IAU Symp. 116, “Luminous Stars and Associations in Galaxies,” Dordrecht: Reidel, p. 139.
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© 1989 Kluwer Academic Publishers
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Leitherer, C., Schmutz, W., Abbott, D.C., Torres-Dodgen, A.V., Hamann, WR., Wessolowski, U. (1989). Atmospheric Models for LBV’s at Minimum and Maximum States. In: Davidson, K., Moffat, A.F.J., Lamers, H.J.G.L.M. (eds) Physics of Luminous Blue Variables. Astrophysics and Space Science Library, vol 157. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-1031-7_43
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DOI: https://doi.org/10.1007/978-94-009-1031-7_43
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6955-7
Online ISBN: 978-94-009-1031-7
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