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تسجيل مستخدم جديدThe radio spectrum of Sgr A*
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We discuss the radio spectrum of Sgr A* index{Sgr A*, radio spectrum} in the frequency range between $approx 1,{rm GHz}$ and $approx 1,000,{rm GHz}$, show that it can be explained by optically thin synchrotron radiation index{Sgr A*, synchrotron radiation, optically thin} of relativistic electrons, and point toward a possible correlation between the spectrum of Sgr A* and larger-scale ($la 50,{rm pc}$) radio emission from the Galactic Center index{Galactic Center} region.
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We demonstrate that there is only one physical process required to explain the spectrum and the variability of the radio source at the dynamical center of our Galaxy, Sgr A*, in the frequency range from $approx$1 to $approx$1000 GHz, namely optically
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