Hostname: page-component-848d4c4894-pjpqr Total loading time: 0 Render date: 2024-06-27T02:27:28.048Z Has data issue: false hasContentIssue false

Atmospheric models for LBV’s at minimum and maximum states

Published online by Cambridge University Press:  12 April 2016

Claus Leitherer
Affiliation:
Joint Institute for Laboratory Astrophysics University of Colorado and National Bureau of Standards
Werner Schmutz
Affiliation:
Joint Institute for Laboratory Astrophysics University of Colorado and National Bureau of Standards
David C. Abbott
Affiliation:
Joint Institute for Laboratory Astrophysics University of Colorado and National Bureau of Standards
Ana V. Torres-Dodgen
Affiliation:
Joint Institute for Laboratory Astrophysics University of Colorado and National Bureau of Standards
Wolf-Rainer Hamann
Affiliation:
Institut fuer Theoretische Physik and Sternwarte der Universitaet, Universitaet Kiel
Ulf Wessolowski
Affiliation:
Institut fuer Theoretische Physik and Sternwarte der Universitaet, Universitaet Kiel

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Section II: Poster Papers, A Brief List of Catalogs, and Index
Copyright
Copyright © Kluwer 1989

References

Appenzeller, I. (1986) in IAU Symp. 116, “Luminous Stars and Associations in Galaxies,” Dordrecht: Reidel, p. 139.Google Scholar
Davidson, K (1987) Ap. J., 317, 760.Google Scholar
Maeder, A., and Meynet, G. (1987) Astr. Ap., 182, 243.Google Scholar