Hoinga (IMAGE)
Caption
Composite X-ray and radio image of Hoinga (see also Fig.2 and Fig.3). The X-rays discovered by eROSITA are emitted by the hot debris of the exploded progenitor, whereas the radio antennae detect synchrotron emission from relativistic electrons, which are decelerated at the outer remnant layer.
Credit
eROSITA/MPE (X-ray), CHIPASS / SPASS / N. Hurley-Walker, ICRAR-Curtin (Radio)
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