Low redshift bal qsos in the eigenvector 1 context
We attempt to characterize the geometry of Broad Absorption Line (BAL)QSOs by studying a low redshift sample of 12 sources. We find that the majorityof these sources are Population A quasars as defined in Sulentic et al. (2000a,broad H B FWHM 4000 km s_1). A possible correlation between terminal ve...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , , , , , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2006
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57142104 |
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