标题： 吸积盘风引起的能谱软化 显示英文标题

标题： Spectral Softening due to Winds in Accretion Disks

摘要： 当吸积流具有正比能量时，可能会产生丰富的风。 风会从盘的内区耗散物质，并使该内区在光学上变得更薄。 由于此区域内电子较少，软光子更容易通过康普顿化来处理，这些软光子是从更远处的开普勒盘截获的。 我们提出了吸积盘风的一个自洽图像，并展示了流出的风如何使盘的光谱变软。 显示英文摘要

摘要： Accretion flows may produce profuse winds when they have positive specific energy. Winds deplete matter from the inner region of the disk and makes the inner region thinner, optically. Since there are fewer electrons in this region, it becomes easier to Comptonize this part by the soft photons which are intercepted from the Keplerian disk farther out. We present a self-consistent picture of winds from an accretion disk and show how the spectra of the disk is softened due to the outflowing wind.