论文标题
潮汐结构中恒星形成部位
Sites of star formation in the tidal structures
论文作者
论文摘要
我们简要审查了在不同交互系统中观察到的恒星形成站点的当前研究结果：ARP 270，ARP 194，ARP 194，ARP 305，NGC 4656和NGC 90。观察结果是在Sao Ras中与Scoprpio-2 plemographs sao Ras中的6米望远镜BTA进行的。在不同系统中，恒星形成岛的特性，它们的质量，动力学，化学丰度，可能的命运和机制启发了恒星形成。
We give a short review of the current results of studying of star formation sites observed beyond the main discs of galaxies in different interacting systems: Arp 270, Arp 194, Arp 305, NGC 4656 and NGC 90. The observations were carried out at the 6-meter telescope BTA in SAO RAS with the SCOPRPIO-2 spectrograph. The properties of star forming islands, their mass, dynamics, chemical abundances, their possible fate and the mechanisms inspiring star formation, appear to be different in different systems.
