Type 1 AGN Unification
| dc.creator | Elvis, Martin | |
| dc.date | 2001-09-27 | |
| dc.date.accessioned | 2026-07-07T02:00:22Z | |
| dc.date.available | 2026-07-07T02:00:22Z | |
| dc.description | The model I recently proposed for the structure of quasars offers to unify the many aspects of Type 1 AGN: emission lines, absorption lines and reflection features. This makes the model heavily overconstrained by observation and readily tested. Here I first outline the model, and then concentrate on how the model answers objections raised since publication - with many of the tests being reported at this meeting. I then begin to explore how these and future tests can discriminate between this wind model and 3 well-defined alternatives. | |
| dc.description | 12 pages, 3 figures. To be published in `Issues in the Unification of AGN' (Elba May 2001) eds. R. Maiolino, A. Marconi and N. Nagar (ASP Conf. Series) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0109513 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0109513 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3410 | |
| dc.subject | Astrophysics | |
| dc.title | Type 1 AGN Unification | |
| dc.type | text |