Fig. 10.
Left: effect of the thermal electron density (determined by the EM) on low-frequency spectra of starburst galaxies seen edge-on. The thermal and nonthermal emitting gases are fully mixed with a constant 10% thermal fraction at 1.4 GHz (to be compared with the analytical model of Condon et al. (1991). Right: similar model applied for a galaxy seen at a different viewing angle with Ne = 80 cm−3.
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