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On the evolutionary status of the WR-type PNN
Published online by Cambridge University Press: 25 May 2016
Extract
Some observed parameters of planetary nebulae with H–deficient (mostly WR–type) nuclei (PNN) are compared to those of H–rich ones and to theoretical predictions from the born again scenario. An example is shown in Fig. 1
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- V. From AGB to Planetary Nebulae
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- Copyright © Kluwer 1997
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