KINEMATICS FROM SPECTRAL LINES FOR AGN OUTFLOWS BASED ON TIME-INDEPENDENT RADIATION-DRIVEN WIND THEORY
We build a bulk velocity-dependent photoionization model of the warm absorber of the Seyfert 1 galaxy NGC 3783. By adopting functional forms for the velocity of the flow and its particle density with radius, appropriate for radiationdriven winds, we compute the ionization, the temperature, the line...
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| Vydáno v: | Revista Mexicana de Astronomía y Astrofísica |
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| Hlavní autor: | |
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
Universidad Nacional Autónoma de México
2011
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| Témata: | |
| On-line přístup: | https://www.redalyc.org/articulo.oa?id=57120957017 |
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