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Binary Nuclei of Planetary Nebulae
Published online by Cambridge University Press: 22 September 2016
Extract
In view of the spectral similarity and the probable evolutionary relation between certain planetary nebulae (PN) and other objects that are generally binaries (symbiotic stars, Be stars, or slow novae), it is probable that many nuclei of PN are double.
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- Session IV: The Central Stars of Planetary Nebulae
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- Copyright © Reidel 1978
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