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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. 4.

On‐SNR spectra of DA 530 (black) and the local background (red). Also shown are the best‐fit model of the on‐SNR spectrum (solid lines), consisting of the free‐﹩N_{\mathrm{H}\,}﹩ vpshock model (see Table 1; diffuse emission) and a power law (Γ ~ 2; sky background). The two individual components are also plotted separately with dashed lines. The residuals of the fit are shown at the bottom.

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