Deciphering the radio–star formation correlation on kpc scales - III. Radio-dim and bright regions in spiral galaxies

Open Access

Fig. I.4.

NGC 4501 model log(radio/SFR)–FP (left panels) and log(radio/SFR)–PI relations (right panels). The upper panels correspond to Fig. 8. Lower panels: addition of a regular field component B_reg = 12 μG in regions of enhanced model polarized intensity (cf. Fig. 9).

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