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IONIZED GAS KINEMATICS AT HIGH RESOLUTION. V. [Ne II], MULTIPLE CLUSTERS, HIGH EFFICIENCY STAR FORMATION, AND BLUE FLOWS IN HE 2–10

  • Authors: Sara Beck, Jean Turner, John Lacy, and Thomas Greathouse

2015 The Astrophysical Journal 814 16.

  • Provider: AAS Journals

Caption: Figure 8.

Channel maps of the W emission region at velocities from the line peak through the “blue bump.” The panes are labeled by velocity and are spaced by 2 pixels, less than one resolution element. Contours are ﹩{2}^{n/2}\times 7\times {10}^{-3}\;\mathrm{erg}{({\rm{s}}\;{\mathrm{cm}}^{-1}{\mathrm{cm}}^{2}\;\mathrm{sr})}^{-1}.﹩

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