Wang, QD2024-04-262024-04-262006-01-01https://doi.org/10.1088/1742-6596/54/1/020https://hdl.handle.net/20.500.14394/2658<p>This is the pre-published version harvested from ArXiv. The published version is located at <a href="http://iopscience.iop.org/1742-6596/54/1/020/">http://iopscience.iop.org/1742-6596/54/1/020/</a></p>About 2 million seconds of Chandra observing time have been devoted to the Galactic Center (GC), including large-scale surveys and deep pointings. These observations have led to the detection of about 4000 discrete X-ray sources and the mapping of diffuse X-ray emission in various energy bands. In this review, I frst summarize general results from recent studies and then present close-up views of the three massive star clusters (Arches, Quintuplet, and GC) and their interplay with the Galactic nuclear environment.Astrophysics and Astronomyarticle