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Revelations in our own backyard: Chandra's unique Galactic Center discoveries

机译:我们自己后院的启示:钱德拉独特的银河中心发现

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Before the launch of Chandra, our Galactic Center supermassive black hole, Sgr A~*, had never been positively identified outside the radio bands. A great deal has changed in the past decade, starting with the discovery that our own backyard harbors a very weak, yet clearly active, galactic nucleus. I will review how this revelation has been a boon for accretion studies around black holes in general and has helped us place our own Galaxy in context within the active galactic nuclei (AGN) zoology. Chandra's exquisite resolution has also unveiled entirely new populations of faint sources and transients, as well as regions of extreme gas dynamics and hints of prior, more typical AGN-like activity in our Galactic Center.
机译:在钱德拉发射之前,我们的银河系中心超大质量黑洞Sgr A〜*在广播频段之外从未得到过肯定的识别。在过去的十年中,发生了许多变化,从发现我们自己的后院拥有一个非常脆弱但明显活跃的银河核开始。我将回顾一下这一发现如何对围绕黑洞的吸积研究大有裨益,并帮助我们将自己的银河置于活跃的银河系原子核(AGN)动物学的背景中。钱德拉(Chandra)的出色分辨率还揭示了全新的微弱源和瞬变种群,以及极端气体动力学区域以及我们银河中心存在先前,更典型的类似于AGN的活动的迹象。

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