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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 6.

Shock-excited molecular hydrogen in the southern shell of the HB 3 SNR (see Figure 5 and the exact location is marked as a white box). Palomar WIRC narrow-band image (a) and Spitzer 4.5 μm (b) and 3.6 μm (c) images centered on R.A. 2h17m46.7ˢ and decl. +61°52′34.1″ (J2000) with an FOV of 8.8′ × 8.4′. The diffuse emission in the WIRC H2 2.12 μm image ranges 0.179–1.3 MJy sr−1 (∼1.91–13.9 × 10−6 erg s−1 cm−2 sr−1). The emission in the Spitzer 4.5 and 3.6 μm images ranges 0.3–1.4 (typical background is 0.2) MJy sr−1 and 0.44–0.83 (0.35) MJy sr−1, respectively. The filament positions of D and E (see Table 4) are marked on the image (b).

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