Four Partially Baked Results
| dc.creator | Antonucci, Robert | |
| dc.creator | Whysong, David H. | |
| dc.date | 2002-12-05 | |
| dc.date.accessioned | 2026-07-07T02:06:44Z | |
| dc.date.available | 2026-07-07T02:06:44Z | |
| dc.description | D Whysong and I have been carrying out a mid-IR survey of 3C radio galaxies to see which have IR-excesses, interpretable as hidden Type-1 AGN. Mostly due to relentless bad weather, we have a modest collections of observations so far. However, we can say with confidence that some radio galaxies are true kinetic, nonthermal emitters, with negligible energetic contributifrom a visible or hidden Big Blue Bump. To make up for the modest collection of mid-IR observations so far, we also present a new spectropolarimetric discovery regarding the underlying shape of the quasar Big Blue Bump in the Balmer Edge region, a fairly radical view of quasar reddening, and a bit of Keck adaptive optics data on Cygnus A and the ultraluminous infrared galaxy NGC6240. | |
| dc.description | 8 pages, 1 figure. To be published in ASP conference proceedings, "Active Galactic Nuclei: from Central Engine to Host Galaxy" | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0212143 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0212143 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5463 | |
| dc.subject | Astrophysics | |
| dc.title | Four Partially Baked Results | |
| dc.type | text |