Hostname: page-component-5c6d5d7d68-lvtdw Total loading time: 0 Render date: 2024-08-06T11:27:57.300Z Has data issue: false hasContentIssue false
  • English
  • Français

Diagnostic Diagrams for Planetary Nebulae and Symbiotic Stars

Published online by Cambridge University Press:  07 August 2017

A. Gutierrez-Moreno ,
H. Moreno  and
G. Cortes
A. Gutierrez-Moreno
Affiliation:
Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Chile
H. Moreno
Affiliation:
Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Chile
G. Cortes
Affiliation:
Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Chile

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.

One of us (Gutiérrez-Moreno 1988) presented some time ago a preliminary version of two diagrams for separating planetary nebulae (PN) from symbiotic stars (SS); tnese diagrams are based on the strength of [O III] lines λλ4363, 5007. Now a new version is presented, which includes more objects and uses measured total intensities corrected by reddening.

Type
IV. Planetary Nebulae Connection: Evolution from the AGB
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 403
Copyright
Copyright © Kluwer 1993 

References

Gutiérrez-Moreno, A. 1988, in “Progress and Opportunities in Southern Hemisphere Optical Astronomy”. CTIO 25th Anniversary Symposium”, eds. Blanco, V.M. and Phillips, M.M. (Utah: Brigharn Young University), A.S.P. Conference Series, 1, 12.Google Scholar