Formation and evolution of Globular Clusters

目前，我正在使用第一个十亿年(FiBY)计划的模拟来研究球状星团的形成和演化。我正在使用对球状星团的局部宇宙观测来完善一套标准，这些标准可以用来在模拟中识别它们和原始球状星团。一旦确定了候选者，我就研究它们的全局和平均性质，以便与目前关于它们形成和演化的理论进行比较，并找到在高红移时可以观察到的性质。未来的目标将是研究中等质量黑洞的形成，并确定球状星团是否有可能容纳它们。

Currently, I am using the simulations from the First Billion years (FiBY) Project to look into the formation and evolution of Globular Clusters. I am using local universe observations of Globular Clusters to refine a set of criteria which can be used to identify them and proto-globulars in the simulations. Once candidates have been identified I then study their global and average properties in order to compare with current theories about their formation and evolution as well as finding properties that could be observed at high redshift. The future aim will be to look into the formation of Intermediate Mass Black Holes and to determine whether Globular Clusters could potentially host them.