“School of Astronomy”
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| Paper IPM / Astronomy / 17006 |
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Resolved maps of the thermal and nonthermal radio continuum (RC) emission of distant galaxies are a powerful tool for understanding the role of the interstellar medium (ISM) in the evolution of galaxies. We simulate the RC surface brightness of present-day star forming galaxies in the past at 0.15 Download TeX format |
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