Modeling mm - to X - ray flare emission from SgrA *


Context. We report on new modeling results based on the mm-to X-ray emission of the SgrA* counterpart associated with the massive ∼4×10 6 M ⊙ black hole at the Galactic Center. Aims. We investigate the physical processes responsible for the variable emission from SgrA*. Methods. Our modeling is based on simultaneous observations carried out on 07 July, 2004… (More)


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