Formation and evolution of Globular Clusters

目前，我正在使用第一个十亿年（FiBY）项目的模拟来研究球状星团的形成和演化。我正在使用球状星团的局部宇宙观测来改进一套标准，这些标准可以用来在模拟中识别它们和原球状星团。一旦候选人已经确定，我然后研究他们的全球和平均性能，以比较与当前的理论，它们的形成和演化，以及寻找可以观察到的高红移的属性。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.