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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. 6.

ACIS‐I spectrum of the central extended feature together with the best‐fit power‐law model with fixed ﹩N_{\mathrm{H}\,}﹩ = 5.7 × 1021 cm−2 and Γ = 1.6. The counts are grouped to have a count‐to‐noise ratio greater than 3 per bin.

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