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Parameter identification – a new way of assessing errors in stellar atmosphere analysis
Published online by Cambridge University Press: 25 May 2016
Abstract
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For the consistent and objective determination of stellar parameters and corresponding errors a constrained minimization approach is described which allows to take additional non-spectroscopic information into account and assures that the atmospheric structure equations are always fulfilled.
- Type
- Stellar Atmospheres
- Information
- Copyright
- Copyright © Kluwer 1997
References
Bock, H.-G.
1981, in: Modelling of Chemical Reaction Systems (Ebert, , Deuflhard, , Jäger, , eds.), Springer Series Chemical Physics 18, 102
CrossRefGoogle Scholar
Kuhn, H. W., Tucker, A. W.
1951, in: Proc. of the Second Berkeley Symposion on Mathematical Statistics and Probability, Neyman, J. (ed.), University of California Press
Google Scholar
Wehrse, R. (ed.) 1990, Accuracy of Element Abundances from Stellar Atmospheres, Lecture Notes in Physics 359, Springer Verlag
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