Iron abundance in galactic H II regions
Some recent results point to a possible discrepancy between the Fe abundance in M42 as derived from theemission of the di erent Fe ions, but it is argued that the uncertainties are currently too high to decidewhether the discrepancy is real. The results of a recent analysis of the Fe abundance in 7...
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| Udgivet i: | Revista Mexicana de Astronomía y Astrofísica |
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| Hovedforfatter: | |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
Universidad Nacional Autónoma de México
2002
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| Online adgang: | https://www.redalyc.org/articulo.oa?id=57112014 |
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