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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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| Foilsithe in: | Revista Mexicana de Astronomía y Astrofísica |
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| Main Authors: | , , , |
| Formáid: | Artigo |
| Teanga: | Inglês |
| Foilsithe: |
Universidad Nacional Autónoma de México
2002
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| Ábhair: | |
| Rochtain Ar Líne: | https://www.redalyc.org/articulo.oa?id=57112036 |
| Clibeanna: |
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