Article contents
On the evolutionary status of the WR-type PNN
Published online by Cambridge University Press: 25 May 2016
Extract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
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
- Type
- V. From AGB to Planetary Nebulae
- Information
- Copyright
- Copyright © Kluwer 1997
References
- 1
- Cited by