Figure 16 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 16.

The best CO(3-2) line profile predicted from our shock model, compared to observations for the S1 position (top panel), the S2 position (middle panel), and the B1 position (bottom panel). The profile intensity is normalized to the observations. The line emission at V_lsr ∼ 0 km s⁻¹ is from gas in the line of sight and unrelated to HB 3.

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