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| Spectra and variability from black hole accretion flows |
| 2010-06-25 | 编辑： | 【大 中 小】【打印】【关闭】 |
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Speaker: Prof. Chris Done (Durham University, UK)
Time: 2:00pm; June 25
Location: Middle Conf. Room; 3rd floor
Abstract:
I will outline how the changes in energy spectra and power spectra seen in galactic black hole can be understood in the truncated disc/hot inner flow model, and how these models give us a starting point to scale up to the supermassive black holes in AGN.
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