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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 3.

WISE four-color mosaic of HB 3 at 3.4 (in blue), 4.6 (in green), 12 (in orange), and 22 μm (in red). The 4.6 μm image is dominated by molecular hydrogen and highlights interacting regions between the SNR and molecular clouds. The image is centered on R.A. 2h17m22.6ˢ and decl. + 62° 37﹩{}^{{\prime} }39\buildrel{\prime\prime}\over{.} 9﹩ (J2000) with a field of view (FOV) of 103′ × 120′. The exact coordinates of the same images are given in Figure 5.

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