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Temperatures of Central Stars of Planetary Nebulae
Published online by Cambridge University Press: 07 August 2017
Extract
The temperature of Central Stars of Planetary Nebulae (CSPN) is one of the most important parameters for a better understanding of their evolution, their properties and those of the surrounding photoionized nebula. It is an elusive quantity to derive though, because CSPN are generally faint objects and their spectrum is often heavily contaminated by nebular continuum emission.
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- II. Highlights on the Nuclei
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- Copyright © Kluwer 1993
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