Fig. 14.

Ranges of the modelled global spectrum of M 51-like galaxy as affected by increasing and decreasing best-fit model parameters ,
, and
by ±20%. Black solid circles denote literature data used during the modelling and the interpolated flux density at 150 MHz from the MSSS survey. For the sake of completeness, the data from individual MSSS sub-bands are also shown (brown rectangles).
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