The origin and physical mechanism of the ensemble Baldwin effect
| dc.creator | Dong, Xiaobo | |
| dc.creator | Wang, Jianguo | |
| dc.creator | Wang, Tinggui | |
| dc.creator | Wang, Huiyuan | |
| dc.creator | Fan, Xiaohui | |
| dc.creator | Zhou, Hongyan | |
| dc.creator | Yuan, Weimin | |
| dc.creator | Long, Qian | |
| dc.date | 2009-03-04 | |
| dc.date | 2009-03-29 | |
| dc.date.accessioned | 2026-07-07T12:57:18Z | |
| dc.date.available | 2026-07-07T12:57:18Z | |
| dc.description | We have conducted a systematic investigation of the origin and underlying physics of the line--line and line--continuum correlations of AGNs, particularly the Baldwin effect. Based on the homogeneous sample of Seyfert 1s and QSOs in the SDSS DR4, we find the origin of all the emission-line regularities is Eddington ratio (L/Ledd). The essential physics is that L/Ledd regulates the distributions of the properties (particularly column density) of the clouds bound in the line-emitting region. | |
| dc.description | to appear in the proceedings of "The Starburst-AGN Connection Conference",ASP Conference Series. Ver2: An appendix of ``Not Baldwin Effect, but ell Effect?'' is added, with two more figures to unveil the nature of the Baldwin effect of AGNs | |
| dc.identifier | https://arxiv.org/abs/0903.0698 | |
| dc.identifier | http://arxiv.org/abs/0903.0698 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/224883 | |
| dc.subject | Astrophysics of Galaxies | |
| dc.title | The origin and physical mechanism of the ensemble Baldwin effect | |
| dc.type | text |