Radio Investigations of the Galactic Center Region

位于洛杉矶的加州大学的马克·莫里斯博士， 将对银河系的核心进行观测研究 在无线电波的波长。 在几年的观察中， 非常大的阵列，PI和他的同事们已经收集了一个非常大的阵列， 关于银河系中心的大量数据，他们已经做出了 几项发现强调了 银河系内部的磁场 他们目前 研究人员继续这些研究与密集的计算工作 充分发挥现有数据库的潜力， 新的观察结果，以澄清负责的物理过程 独特的观察现象学。 银河系中心提供了一个近距离的例子， 活动星系核 因此，它可以给我们 对过程的新见解，也发生在更活跃的 Seyfert和类星体现象。 使用新的仪器，如 超大型阵列和新的数据分析功能，如 在超级计算机上进行图像处理，我们能够研究 我们银河系中心的结构，前所未有的详细。 莫里斯博士一直是领导者，在完善我们的知识， 银河中心

Dr. Mark Morris, at the University of California, Los Angeles, will carry out observational research on the nucleus of our Galaxy at radio wavelengths. During several years of observing with the Very Large Array, the PI and his colleagues have gathered a very extensive body of data on the Galactic Center, and they have made several discoveries which highlight the importance of strong magnetic fields in the inner regions of the Galaxy. Their current research continues these studies with intensive computational work to realize the full potential of the existing data base and with new observations to clarify the physical processes responsible for the unique observed phenomenology. The Galactic Center provides a close-up example of a moderately active galactic nucleus. As such it can be expected to give us new insights into processes which also occur in the more active Seyfert and quasar phenomena. With new instrumentation such as the Very Large Array and new data analysis capabilities such as image processing on supercomputers, we are able to study the structure of the center of our Galaxy in unprecedented detail. Dr. Morris has been a leader in refining our knowledge about the Galactic Center.