The coronal line spectrum of the brightest seyfert galaxies as seen by iso
The ISO coronal line spectrum of a sample of the brightest known Seyfertgalaxies is presented and modeled. ISO observations of [O IV] 25.9 , [Ne V] 14.3, [Mg VIII] 3.02 and [Si IX] 2.58 lines are presented; their relationship withthe ionizing spectrum from 50 to 300 eV is investigated. Pure photoi...
Tallennettuna:
| Julkaisussa: | Revista Mexicana de Astronomía y Astrofísica |
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| Päätekijät: | , |
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
Universidad Nacional Autónoma de México
2000
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| Aiheet: | |
| Linkit: | https://www.redalyc.org/articulo.oa?id=57100981 |
| Tagit: |
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