Figure 11 from Shocked Molecular Hydrogen and Broad CO Lines from the Interacting Supernova Remnant HB 3

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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 11.

12 m CO(1-0) spectrum of HB 3 B1 (CO(3-2) spectrum is shown in Figure 10(a)) with an offset of (+10,+20) shows a broad CO line with an FWHM of 18 km s⁻¹ with high signal to noise. The numbers shown on the upper side are frequencies in megahertz.

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