Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-29T06:40:58.679Z Has data issue: false hasContentIssue false
  • English
  • Français

Planetary Nebulae by the Strong [NII] Emission Lines

Published online by Cambridge University Press:  07 August 2017

L. N. Kondratjeva
L. N. Kondratjeva*
Affiliation:
Astrophysical Institute of Kazakh Academy of Sciences, Kamenskoje Plato, 480068 Alma-Ata, Kazakhstan

Abstract

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.

The sample of planetaries with the strong [NII] emission lines are analysed. All available parameters are discussed. The enrichments of all elements and the tendency to rather low surface brightness of ne bulae in Hβ flux are remarked. The deficiency of hydrogen in envelopes is proposed as the possible reason of observational spectra.

Type
III. Highlights on the Nebulae
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 195
Copyright
Copyright © Kluwer 1993