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Molecular Gas in the Outflow of the Small Magellanic Cloud

  • Authors: Enrico M. Di Teodoro, N.M. McClure-Griffiths, C. De Breuck, L. Armillotta, N.M. Pingel, K.E. Jameson, John M. Dickey, M. Rubio, S. Stanimirović, and L. Staveley-Smith

2019 The Astrophysical Journal Letters 885 L32.

  • Provider: AAS Journals

Caption: Figure 3.

Spectra of the main clumps of 12CO(2 → 1) emission (black line) detected with APEX for SMC-C1 (left panels) and SMC-C2 (right panels). Spectra are integrated over a 0.′7 circular aperture. The velocity range of each detection is highlighted in gray. The narrow emission line at ﹩{V}_{\mathrm{LSR}}\simeq 91\,\mathrm{km}\,{{\rm{s}}}^{-1}﹩ visible in the SMC-C1’s clump 5 spectrum is contaminated from the nearby, spectrally decoupled, clump 4. Light blue histograms denote H I spectra integrated on the same aperture and normalized to the CO peak for a easier visualization.

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