Fig. 3

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Small Magellanic Cloud radio spectrum. The data points (dots) are from Table 4 of For et al. (2018). Left: preferred 1PL model 1 of For et al. (2018; solid line), and best-fitting third-order polynomial (dashed curve; see Table 4). Right: the two-component model (solid curve) that mimics the polynomial includes synchrotron radiation (dot-short-dashed curve) and thermal ff emission (dot-long-dashed curve); the primary and secondary synchrotron contributions are also shown (dashed, dotted curves).
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