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Shocked Molecular Hydrogen and Broad CO Lines from the Interacting Supernova Remnant HB 3

  • Authors: J. Rho, T. H. Jarrett, L. N. Tram, W. Lim, W. T. Reach, J. Bieging, H.-G. Lee, B.-C. Koo, and B. Whitney

2021 The Astrophysical Journal 917 47.

  • Provider: AAS Journals

Caption: Figure 1.

ROSAT PSPC X-ray image (0.3–2.4 keV) superposed on radio contours of HB 3 at 92 cm (320 MHz) from the Westerbork Northern Sky Survey (Landecker et al. 1987). All images have J2000 coordinates. The X-ray image has the intensity range of (0.35–6.4) × 10−3 counts s−1 arcmin−2. The image shows a center-filled X-ray morphology with an inner ring structure. The radio contours are 0.8, 4.9, 8.9, 13, and 17 mJy beam−1.

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