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Non-LTE Model Atmosphere Analysis of Central Stars∗
Published online by Cambridge University Press: 18 September 2017
Extract
This review will be concentrated on the determination of the main atmospheric parameters (Teff, log g, helium abundance) of PN nuclei, and of other subluminous objects, by fitting the observed absorption line profiles with theoretical profiles obtained from non-LTE model atmosphere calculations.
- Type
- Section V: Central Stars of Planetary Nebulae
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- Copyright
- Copyright © Reidel 1983
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