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Planetary Nebulae with Massive Central Stars

Published online by Cambridge University Press:  19 July 2016

R. Tylenda
R. Tylenda*
Affiliation:
Laboratory of Astrophysics, Copernicus Astronomical Center, Chopina 12/18, 87-100 Toruń, Poland

Abstract

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The paper discusses the problem of planetary nebulae with massive nuclei from the point of view of their theoretical evolution and observational appearances. The available data suggest that NGC 2440, 6302, and 7027 have central stars with masses greater than 0.8 M⊙.

Type
VI. Evolution
Information
Symposium - International Astronomical Union , Volume 131: Planetary Nebulae , 1989 , pp. 531 - 538
Copyright
Copyright © Kluwer 1989 

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