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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 7.

Top: the [Ne II] line profile on the E edge of the SE emission region and just off the emission region, with the best fit to the latter. X-axis units are km s−1 and Y-axis units are erg(s cm−1 cm2 sr)−1. Bottom: channel maps labeled by velocity over the velocity region of the 873 km s−1 feature. Contours are ﹩{2}^{n/2}\times 7\times {10}^{-3}\;\mathrm{erg}{({\rm{s}}\;{\mathrm{cm}}^{-1}\;{\mathrm{cm}}^{2}\;\mathrm{sr})}^{-1}.﹩ The spacing between channels is one velocity pixel or one-fourth of a velocity resolution element.

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