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Temperatures of Central Stars of Planetary Nebulae

Published online by Cambridge University Press:  07 August 2017

A. Preite-Martinez*
Affiliation:
Istituto di Astrofisica Spaziale, CP 67, 00044 Frascati, Italy Observatoire de Strasbourg, 11 rue de l'Universitè, 67000 Strasbourg, France

Extract

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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.

Type
II. Highlights on the Nuclei
Copyright
Copyright © Kluwer 1993 

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