[Fe IV] Emission in Ionized Nebulae
I present the results of an analysis of [Fe IV] emission in several ionized nebulae, which is based on new identifications and previous measurements of [Fe IV] lines. The Fe abundances obtained by adding the abundances of the relevant Fe ions (mainly Fe++ and Fe3+) are found to be lower, by factors...
Gorde:
| Argitaratua izan da: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Egile nagusia: | |
| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
Universidad Nacional Autónoma de México
2003
|
| Gaiak: | |
| Sarrera elektronikoa: | https://www.redalyc.org/articulo.oa?id=57101826 |
| Etiketak: |
Etiketarik gabe, Izan zaitez lehena erregistro honi etiketa jartzen!
|