The role of inner density waves in fueling galactic nuclei
Astrophysics
2007-05-23 v1
Abstract
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.
Cite
@article{arxiv.astro-ph/0302414,
title = {The role of inner density waves in fueling galactic nuclei},
author = {Eric Emsellem},
journal= {arXiv preprint arXiv:astro-ph/0302414},
year = {2007}
}
Comments
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)'