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...
Gardado en:
| Publicado en: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Autor Principal: | |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
Universidad Nacional Autónoma de México
2011
|
| Assuntos: | |
| Acceso en liña: | https://www.redalyc.org/articulo.oa?id=57120957017 |
| Tags: |
Sen Etiquetas, Sexa o primeiro en etiquetar este rexistro!
|