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Model Atmospheres of Central Stars of PN
Published online by Cambridge University Press: 07 August 2017
Abstract
We review the work done in this field since the time of the Mexico Symposium on PN, five years ago. Although substantial progress has been achieved, a lot of work is still needed, and we pay attention to some remaining problems. We briefly describe some recent results about stellar and nebular properties, obtained with NLTE model atmosphere techniques.
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- II. Highlights on the Nuclei
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- Copyright © Kluwer 1993