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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 6.

TEXES [Ne II] emission in color overlaid on the CO(2-1) SMA channel maps of Santangelo et al. (2009). The panels are labeled by the [Ne II] velocity channel. The SMA channel velocities are within 3 km s−1 of the [Ne II]. The molecular clouds discussed in the text are labeled with Santangelo et al.’s (2009) numbers. The + marks the position of the central nonthermal radio source, posited to be an AGN, in between the eastern and western starforming regions (E and W in the text.) The [Ne II] spectra have been convolved to match the CO(2-1) 2″ beam, and the 5 km s−1 resolution of the CO maps.

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