Abstract—In this work a search was carried out for globular clusters belonging to the Sagittarius (Sgr) tidal stream using the analysis of spatial positions, radial velocities relative to the Galactic Standard of Rest (V_GSR), proper motions and ratio of “age–metallicity” ([Fe/H]) for globular clusters and for stars in the tidal stream. As a result, three categories of globular clusters were obtained: A—most certainly in the stream: Terzan 8, Whiting 1, Arp 2, NGC 6715, Terzan 7, Pal 12; B—kinematic outliers: Pal 5, NGC 5904, NGC 5024, NGC 5053, NGC 5272, NGC 288; C—lowest rank candidates: NGC 6864, NGC 5466, NGC 5897, NGC 7492, NGC 4147.

摘要—在这项工作中，通过分析空间位置，相对于银河静止标准（V _GSR）的径向速度，适当运动和“年龄”比率，对属于射手座（Sgr）潮汐流的球状星团进行了搜索“金属性”（[Fe / H]）用于球状星团和潮汐流中的恒星。结果，获得了三类球状星团：A-最肯定的是在流中：Terzan 8，Whiting 1，Arp 2，NGC 6715，Terzan 7，Pal 12；B-运动异常值：Pal 5，NGC 5904，NGC 5024，NGC 5053，NGC 5272，NGC 288；C级最低候选人：NGC 6864，NGC 5466，NGC 5897，NGC 7492，NGC 4147。