The role of inner density waves in fueling galactic nuclei
| dc.creator | Emsellem, Eric | |
| dc.date | 2003-02-20 | |
| dc.date.accessioned | 2026-07-07T02:07:41Z | |
| dc.date.available | 2026-07-07T02:07:41Z | |
| dc.description | I present here an heterogeneous selection of nearby galaxies in which inner density waves (bars, spirals, m=1 modes) have been observed, and which are presumed to host a supermassive black hole, to illustrate the importance of such inner waves in the fueling of the central 10s of parsecs. | |
| dc.description | 9 pages, 5 figures, (see http below for high res. figures), To appear in "Carnegie Observatories Astrophysics Series, Vol. 1: Coevolution of Black Holes and Galaxies," ed. L. C. Ho (Pasadena: Carnegie Observatories, http://www.ociw.edu/ociw/symposia/series/symposium1/proceedings.html)' | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0302414 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0302414 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5773 | |
| dc.subject | Astrophysics | |
| dc.title | The role of inner density waves in fueling galactic nuclei | |
| dc.type | text |