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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 5.

Highlighting the most prominent regions of shock-excited molecular hydrogen. Bright shocked H2 emission is de-marked with boxes and labels (in cyan). The white box denotes near-IR) H2 imaging with WIRC (see Figure 6 for the southern FOV, and see Figure 7 for the southeastern FOV). The yellow box denotes the FOVs of CO observations (see Figure 9 for the southern FOV, and see Figure 10 for the southeastern FOV).

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