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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 1.

Small Magellanic Cloud (SMC) in Hα emission (MCELS survey; Winkler et al. 2015) in red color scale. The two clouds (SMC-C1 and SMC-C2) detected in H I emission (ASKAP; McClure-Griffiths et al. 2018) and targeted in this work are shown in blue color scale. H I contours (blue) are at ﹩(1.0,2.0)\times {10}^{19}﹩ cm−2 (SMC-C1) and ﹩(1.5,2.5)\times {10}^{19}﹩ cm−2 (SMC-C2). The red box denotes the star formation regions (NGC 371/395) from where the clouds could have been launched.

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