A bi-component spectral analysis of 4 planetary nebulae
Presented here is the analysis of four planetary nebulae which show well{resolved Doppler splitting of their emission lines into distinct spectral components.The red, (R), and blue, (B), components of the spectral lines have been separatelyanalyzed to obtain the reddening, the electron temperature,...
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| Veröffentlicht in: | Revista Mexicana de Astronomía y Astrofísica |
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| Hauptverfasser: | , |
| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
Universidad Nacional Autónoma de México
2001
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| Schlagworte: | |
| Online-Zugang: | https://www.redalyc.org/articulo.oa?id=57101012 |
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