Figure 4 from Turbulent Molecular Gas and Star Formation in the Shocked Intergalactic Medium of Stephan's Quintet

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Turbulent Molecular Gas and Star Formation in the Shocked Intergalactic Medium of Stephan's Quintet

Authors: P. Guillard, F. Boulanger, G. Pineau des Forêts, E. Falgarone, A. Gusdorf, M. E. Cluver, P. N. Appleton, U. Lisenfeld, P.-A. Duc, P. M. Ogle, and C. K. Xu

Guillard et al. 2012 The Astrophysical Journal 749 158.

Provider: AAS Journals

Caption: Figure 4.

Overlay of the CO(1–0), CO(2–1), and CO(3–2) spectra observed in the Stephan's Quintet shock, at the positions Ridge 1. No beam size convolution has been applied. The spectra have been shifted vertically for clarity. The arrows indicate the pre-shock H i velocities for the intruder galaxy and the intra-group medium.

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