Abstract
High-resolution Chandra and XMM-Newton X-ray spectroscopic studies of stellar and supermassive black holes have revealed that these phenomenologically different systems share many common physical characteristics. The observed outflows in the micro-quasar GRS 1915+105, the Seyfert 1 galaxy MCG-6-30-15 and the Seyfert 2 galaxy IRAS 18325-5926 are the focus of this proceeding.
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Lee, J.C. (2005). Black hole systems seen at high spectral resolution: Inflow and outflow. In: Maccarone, T.J., Fender, R.P., Ho, L.C. (eds) Astrophysics and Space Science. Springer, Dordrecht. https://doi.org/10.1007/1-4020-4085-7_8
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DOI: https://doi.org/10.1007/1-4020-4085-7_8
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Online ISBN: 978-1-4020-4085-6
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