对银河系中心超大质量黑洞候选体Sgr A*的VLBI观测研究

位于银河系中央的极其致密的非热射电源Sagittari8us A^*（Sgr A^*），被公认为最佳的超大质量黑洞候选体，其质量约为400万个太阳质量。甚长基线干涉测量（BLBI）技术以其独有的高空间分辩率为我们提供了唯一可以探讨Sgr A^*位于几个史瓦西（Schwarzschild）半径区域内天体物理性质的手段。介绍了对 Sgr A^*的VLBI研究现状和最新进展，着重论述了毫米波和亚毫米波VLBI观测对研究Sgr A^*的辐射区域的真实形状和大小，以及探索其结构随时间变化的重要性。Sgr A^*无疑是检验广义相对论将就的亚亮米波VLBI实验的最佳目标。

VLBI OBSERVATIONS OF SGR A*:A SUPERMASSIVE BLACK HOLE CANDIDATE AT THE GALACTIC CENTRE

There is compelling evidence that the extremely compact non-thermal radio source at the center of our Milky Way Galaxy, Sagittarius A* ( Sgr A*), is a best known supermassive black hole candidate with a dark mass of 4 million solar masses. Very Long Baseline Interferometry (VLBI) technique, with its high-resolution imaging capability, is proved to be the most powerful tool for probing the region of a few Schwarzschild radii of Sgr A*. This paper updates the progress in the VLBI observations of Sgr A*, with the emphasis on the importance of the millimeter and sub-millimeter VLBI observations in the detection of the intrinsic structure of Sgr A* and in our ongoing effort to search for the structural variability. There is no doubt that Sgr A* would be the most important target for the future sub-millimeter VLBI experiment to test the General Relativity.