Fig. 3
Synchrotron and self-Compton models for the synchronous NIR and X-ray flare peak of SgrA* observed on 7 July 2004. The results are shown for the three emission modes (SSC-SSC, SYN-SSC, SYN-SYN) in the particle density/magnetic field plane and in the flux density/source size plane. The grey shaded ellipses and thick arrows are described in the text.
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