Chemical composition of planetary nebulae: including iso results

The method of determining abundances using Infrared Space Observatory spectra is discussed. The results forseven planetary nebula are given. Using these data, a preliminary discussion of their evolution is given.

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Udgivet i:Revista Mexicana de Astronomía y Astrofísica
Main Authors: S. R. Pottasch, D. A. Beintema, J. Bernard Salas, W. A. Feibelman
Format: Artigo
Sprog:Inglês
Udgivet: Universidad Nacional Autónoma de México 2002
Fag:
Física, Astronomía y Matemáticas
ERAL
ISM: ABUNDANCES
STARS: EVOLUTION
ISM: LINES AND BANDS
PLANETARY NEBULAE: GEN
Online adgang:https://www.redalyc.org/articulo.oa?id=57112036
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