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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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發表在:Revista Mexicana de Astronomía y Astrofísica
Main Authors: S. R. Pottasch, D. A. Beintema, J. Bernard Salas, W. A. Feibelman
格式: Artigo
語言:Inglês
出版: Universidad Nacional Autónoma de México 2002
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在線閱讀:https://www.redalyc.org/articulo.oa?id=57112036
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