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Neutral ISM, Lyα, and Lyman-continuum in the Nearby Starburst Haro 11

  • Authors: T. Emil Rivera-Thorsen, Göran Östlin, Matthew Hayes, and Johannes Puschnig

2017 The Astrophysical Journal 837 29.

  • Provider: AAS Journals

Caption: Figure 4.

Si II and other LIS (upper) and Si IV (lower) profiles included in this study. Dashes denote data points masked out due to foreground contamination. Data in this figure have been smoothed to better show the line shapes, but all computations have been carried out on the unsmoothed data. Note the high-velocity component in both Si IV lines, extending out to ∼850 km s−1.

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