Seyfert星系中冲击性外流：影像学视角
天体物理学
2007-05-23 v1
摘要
presented一项搜索Seyfert星系核周围气体呈现冲击特征结构的代表性结果。争议点在于，我们能否识别出这些看似因活跃天体核的外流而产生冲击的区域。此类区域将是未来光谱光度研究的优选目标，以确定冲击在活跃星系核/宿主星系相互作用中的物理作用。
引用
@article{arxiv.astro-ph/9607162,
title = {Shocking Outflows in Seyfert Galaxies: An Imaging Perspective},
author = {Richard Pogge},
journal= {arXiv preprint arXiv:astro-ph/9607162},
year = {2007}
}
备注
4 pages with 2 embedded PostScript figures, uses aspconf.sty, epsf.sty; To appear in "Emission Lines in Active Galaxies: New Methods and Techniques", proceedings of IAU Colloquium 159, Shanghai, June 1996. eds. B.M. Peterson, F.-Z. Cheng, and A.S. Wilson (Astronomical Society of the Pacific: San Francisco)