Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-30T20:58:04.617Z Has data issue: false hasContentIssue false
  • English
  • Français

Binary Nuclei of Planetary Nebulae

Published online by Cambridge University Press:  22 September 2016

Agnès Acker
Agnès Acker*
Affiliation:
Observatoire de Strasbourg, France

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.

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.

Type
Session IV: The Central Stars of Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 76: Planetary Nebulae , 1978 , pp. 209
Copyright
Copyright © Reidel 1978