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The Chandra View of DA 530: A Subenergetic Supernova Remnant with a Pulsar Wind Nebula?

  • Authors: Bing Jiang, Yang Chen, and Q. Daniel Wang

Jiang, Chen, & Wang 2007 The Astrophysical Journal 670 1142.

  • Provider: AAS Journals

Caption: Fig. 7.

Left, 1.4 GHz NRAO VLA Sky Survey intensity map; right, 325 MHz Westerbork Northern Sky Survey intensity map. The scales are linear. The same 0.5–2 keV intensity contours as in Fig. 3, except for the highest level, are overlaid to show the positional correspondence of the PWN candidate (indicated by two tick marks) with the radio source.

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