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Left: Chandra image of the X-ray emitting hot gas plus the HST image of the stars in a z = 0.5 brightest cluster galaxy and cooling flow cluster. Center: the JVLA L band image at 1” resolution, and the VLBA 5 GHz image at 1.4mas x 4.3mas resolution. Right: the HST image of the stars and the JVLA image at 1.4 GHz of the parent galaxy (Ubertosi et al. 2025, ApJ 989, 128).
Figure1-1-4-4.png
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