A Multiwavelength Study Of The Mixed-Morphology Supernova Remnant W28

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We present X-ray images from Chandra and ROSAT along with narrow-band optical images of the mixed-morphology supernova remnant W28. We spatially compare these data with VLA maps that have been previously published in the literature. While the radio observations clearly reveal a non-thermal shell, the ROSAT and Chandra observations confirm that the X-ray emission is centrally concentrated and primarily thermal in origin; the contrasting X-ray and radio morphologies are characteristic of mixed-morphology SNRs. Narrow-band optical images from the Curtis Schmidt telescope at Cerro Tololo International Observatory reveal complex filamentary structure. There is a relative enhancement of [S II] compared to H-alpha in the regions of known shock/cloud interactions and the converse is true in the central X-ray emitting region. Our Chandra image details the shape and extent of the central emission, revealing a bright knotty region approximately 5-10 arcmin in size. Spatially resolved spectroscopy shows that the diffuse X-ray emission has uniform temperature in the regions covered by our Chandra observations, as it typical of other mixed-morphology SNRs. The Chandra data also reveal a hard X-ray point source coincident with the southwestern shell. This hard source is most likely unrelated to W28: we argue that confusing emission from this source may be responsible for spectral variations reported previously for W28 based on prior X-ray observations.

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