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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 12.

Distribution of LSR velocity and the FWHM at different positions of HB 3, including the FWHMs from representative spectra shown in Figures 9 and 10 in addition to those in Table 5. The first component (in red) are broad lines except in the SE (H II) region.

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