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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 4.

Left: the [Ne II] line averaged over the W source, the symmetrized profile made by reflecting the red half of the line, the best single Gaussian fit to the symmetrized data, and the residuals of the original, non-symmetrized data. X-axis units are km s−1 and Y axis units are erg(s cm−1 cm2 sr)−1. Note that the original data and the symmetrized are very similar except in the high noise region around 830 km s−1. Right: the same as the left panel, with another Gaussian appropriate for the “blue bump” added. The formal significance of the second Gaussian is low because of the high noise.

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