Fig. 10
Multi-colour Herschel/SPIRE image of 3C 58 created from images at 510 μm (587 GHz; red), 350 μm (857 GHz; green) and 250 μm (1200 GHz; blue). A white ellipse of 9′ × 5′ diameter shows the size of the radio SNR. The diffuse interstellar medium is mostly white in this image, while the emission within the ellipse is distinctly red, being brightest at 510 μm while the diffuse interstellar medium is brightest at 250 μm. The red, compact source at the centre of the ellipse is coincident with PSR J0205+6449 that is thought to be the compact remnant of the progenitor star.
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