标题： 法布里-珀罗星爆和AGN风成像光谱学 显示英文标题

标题： Fabry-Perot Imaging Spectroscopy of Starburst and AGN Winds

摘要： 到目前为止，对星系风最详细的研究来自于使用射电和法布里-珀罗干涉仪的三维光谱测光观测。 在这里，我们报告了在毛纳基山使用夏威夷成像法布里-珀罗干涉仪（HIFI）和澳大利亚的TAURUS-2系统对附近活动星系和星爆星系进行长期光学调查的最新结果。 这些数据表明，外流非常复杂，能量很高（大多数情况下超过10^{53} ergs），并且最明亮的发射通常似乎与强烈的冲击有关。 星爆星系中的外流物质通常位于气泡的表面或沿着快速从星系平面加速出来的漏斗状风的壁上。 这些风有时相对于宿主星系的极轴是不对称且倾斜的。 在一些天体中可以看到（旋转）盘状物质被卷入的证据。 我们的结果结合了哈勃空间望远镜（HST）、射电和X射线数据，并在8米级望远镜对遥远星系未来调查的背景下进行了讨论。 显示英文摘要

摘要： To date, the most detailed studies of galactic winds have come from 3-D spectrophotometric observations with radio and Fabry-Perot interferometers. Here, we report the latest results from a long-term optical survey of nearby active and starburst galaxies with the Hawaii Imaging Fabry-Perot Interferometer (HIFI) at Mauna Kea and the TAURUS-2 system in Australia. These data reveal that the outflows are highly complex, highly energetic (> 10^{53} ergs in most cases), and the brightest emission often appears to be associated with strong shocks. The outflowing material in the starburst galaxies generally lies on the surface of bubbles or along the walls of funnel-shaped winds rapidly accelerating out of the galactic plane. These winds are sometimes lop-sided and tilted with respect to the polar axis of the host galaxy. Evidence for entrainment of (rotating) disk material is seen in some objects. Our results are combined with HST, radio and X-ray data and discussed in the context of future surveys of distant galaxies on 8-meter class telescopes.