ar X iv : a st ro - p h / 05 11 59 0 v 1 1 9 N ov 2 00 5 submitted
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چکیده
We model thermal X-ray emission from the accreting supermassive black hole Sagittarius A* at the Galactic Center. For the region inside 1.5 of the center, we use a generalized radiatively inefficient accretion flow (RIAF) model, and for the region out to 10 we use published models of the ambient hot gas. We calculate the equivalent widths of Hydrogen-like and Helium-like emission lines of various elements, notably iron. We predict that a strong Helium-like iron line with an equivalent width ∼ 1 keV should be emitted by both the external medium and the RIAF. The equivalent width in the external medium is sensitive to the metallicity Z of the gas as well as the mean temperature. For reasonable choices
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تاریخ انتشار 2005