Fig. 12.
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Left: Integrated synchrotron emission for NGC 3125 with the free–free absorption fit. The turnover in the spectrum can be an attribute of free–free absorption processes in the galaxy. Additionally, for NGC 3125 there may be some flux loss at 2740 MHz due to the use of only long baselines. Therefore the data point marked in dark red and shown as a lower limit, does not contribute to the fit. Right: Integrated synchrotron emission for IC 4662 with the free–free absorption fit. The 4.8 and 8.64 GHz have not been taken into account for the fit. A small turnover point have been observed.
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