The Ionized Interstellar Medium in Irregular Galaxies

大的电离气体环和细丝已经被观察到躺在 在一些不规则星系的HII区边界之外。 这些特征的起源和电离源尚不清楚， 但它们可能参与了星星形成的反馈过程， 在整个反馈过程中， 他们所观察到的。 首席研究员，探索 这些结构的物理性质，以阐明它们在星星中的作用 形成活动。

Large loops and filaments of ionized gas have been observed lying outside the boundaries of HII regions in some irregular galaxies. The origin and source of ionization of these features is not known, but they could be involved in star formation feedback processes and in dispersing heavy elements throughout feedback processes and in which they are observed. The Principal Investigator, explore the physical nature of these structures to elucidate their role in star formation activity.