我们计划用最新的观测资料对最新证认的M31和M33晕中的球状星团进行研究：（1）给出这些球状星团在同一系统（BATC测光系统）下的15色中带滤光片的测光资料。利用BATC系统的几个颜色和金属丰度有很好相关性的关系，求出它们的金属丰度，进而利用最新的星族合成模型求出它们的年龄，即准确地确定它们的星族成份；（2）利用高分辨率的哈勃成像和最新的动力学模型得到这些球状星团的动力学参数；（3）和银河系晕中的球状星团，以及M31和M33盘中的球状星团的星族成份及动力学结构进行统计研究，发现它们有何异同，对它们的形成和演化进行细致的研究；（4）结合我们原来的工作，我们将给出M31和M33中所有的已确认的星团在BATC系统下的15色中带波段的测光数据，同时我们得到无缝的M31 50平方度和M33 6平方度的15色中带波段的图像资料，这对将来整体研究近邻星系中的星族成份及星系的形成和演化具有很重要的价值。

We plan to study newly-detected globular clusters in the halos of M31 and M33 based on the newest observed data from 15 BATC intermediate-band filters and images from HST, using the newest stellar population synthesis models and dynamics models. (1) We will provide photometric data in 15 intermediate-band filters of BATC system. Based on the relations between colors in the BATC system and metallicity for globular clusters, we will determine their metallcities, and then their ages by using the newest stellar population synthesis models. So, we can determine stellar populations for these globular clusters in the halos of M31 and M33. (2) We will determine their structural parameters based on the HST images and newest dynamics models. (3) We will compare the stellar populations and structural parameters between them and the counterparts in the halo of the Wilky Way and in the disks of M31 and M33, and will study their formation and evolution in detail. (4) Combined our previous works, we will provide photometric data in 15 intermediate-band filters of BATC system for all the star clusters in M31 and M33. At the same time, we will provide the contiguous images covering 50 square degrees from M31's center and 6 square degrees from M33's center, which are very important for studying the stellar populations and formation and evolution of a galaxy in the Local Group galaxy.