Abstract
Because of its proximity the Center of the Milky Way is a unique laboratory for studying physical processes that are thought to occur generally in galactic nuclei. The central parsec of our Galaxy is known to contain a dense and luminous star cluster, as well as several components of neutral, ionized and extremely hot gas. For two decades, evidence has been mounting that the Galactic Center harbors a concentration of dark mass (3-4 million solar masses) associated with the compact radio source SgrA* (diameter about 10 light minutes), located at the center of the nuclear star cluster. SgrA* has long thought to be a supermassive black hole. High resolution observations offer the unique opportunities of stringently testing the black hole paradigm and of studying stars and gas in the immediate vicinity of a black hole, at a level of detail that will never be accessible in any other galactic nucleus.
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Genzel, R., Ott, T., Eckart, A., Schödel, R., Alexander, T. Inward Bound: High Resolution AO Observations of the Galactic Center. In: Brandner, W., Kasper, M.E. (eds) Science with Adaptive Optics. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10828557_48
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DOI: https://doi.org/10.1007/10828557_48
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Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-25034-0
Online ISBN: 978-3-540-31605-3
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