| Autor: |
Zhang, S.-Y., Bian, W.-H., Huang, K.-L., Zhang, S.-Y., Bian, W.-H., Huang, K.-L. |
| Zdroj: |
Astronomy and Astrophysics; September 2008, Vol. 488 Issue: 1 p113-116, 4p |
| Abstrakt: |
Aims. Type II active galactic nuclei (AGNs) with polarimetric broad emission lines provided strong evidence for the orientation-based unified model for AGNs. We want to investigate whether the polarimetric broad emission lines in type II AGNs can be used to calculate their central supermassive black hole (SMBH) masses, like that for type I AGNs. |
| Databáze: |
Supplemental Index |
| Externí odkaz: |
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