Hostname: page-component-848d4c4894-jbqgn Total loading time: 0 Render date: 2024-06-16T04:56:37.801Z Has data issue: false hasContentIssue false
  • English
  • Français

Spectroscopy of new Planetary Nebulae close to the galactic center

Published online by Cambridge University Press:  25 May 2016

G.C. Van de Steene  and
G. H. Jacoby
G.C. Van de Steene
Affiliation:
1European Southern Observatory
G. H. Jacoby
Affiliation:
1European Southern Observatory

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.

Planetary Nebulae (PN) are bright emission line objects, observable at large distances throughout the Galaxy. They serve as probes of abundance gradients and chemical enrichment history of the ISM.

Type
VII. Planetary Nebulae in the Galactic Context
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 414
Copyright
Copyright © Kluwer 1997