The Gaseous Environment of Seyfert Galaxies
| dc.creator | Mundell, C. G. | |
| dc.date | 2000-12-11 | |
| dc.date.accessioned | 2026-07-07T01:56:58Z | |
| dc.date.available | 2026-07-07T01:56:58Z | |
| dc.description | The VLA has been used to image HI in a heterogeneous sample of nine Seyferts as part of a continuing investigation of the role of galactic host gas in the triggering and fuelling of nuclear activity. Where previous single-dish observations indicated complex, poorly understood kinematics, improved angular resolution and sensitivity reveal tidal tails and intragroup gas, distinguish dwarfs from main disks and resolve non-linear gas dynamical features such as shocks in bars. Seyferts may be abnormally gas-rich, but a larger, statistically significant comparison of HI properties of normal and active galaxies is now required. | |
| dc.description | 3 pages, 2 figures, to be published the in ASP conference proceedings of "Gas and Galaxy Evolution", eds. J.E. Hibbard, M.P. Rupen & J.H. van Gorkom | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0012230 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0012230 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/2204 | |
| dc.subject | Astrophysics | |
| dc.title | The Gaseous Environment of Seyfert Galaxies | |
| dc.type | text |