内密度波在喂给银河系核源中的作用
天体物理学
2007-05-23 v1
摘要
我在此呈现一组近距离银河系中观察到的内部密度波(栏、螺旋、m=1 模式)的异构选取样本，这些样本被认为包含超大质量黑洞，以说明此类内部波在喂给距离银河系核源几十尺距的重要性。
引用
@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}
}
备注
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)'