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...
Tallennettuna:
| Julkaisussa: | Revista Mexicana de Astronomía y Astrofísica |
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| Päätekijät: | , , , , , , |
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
Universidad Nacional Autónoma de México
2006
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| Aiheet: | |
| Linkit: | https://www.redalyc.org/articulo.oa?id=57142104 |
| Tagit: |
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