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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 3.

Effective resolution estimate. Upper left: Haro 11 in UV-continuum, data from Östlin et al. (2009) and Hayes et al. (2009). Data are shown on a square root scale and cut levels set for best detail. Inset in blue is the COS aperture covering the region surrounding knot B in the terminology of Vader et al. (1993). N is up, E is left. Upper right: extracted, throughput-corrected in-aperture image, rotated so horizontal corresponds to the dispersion direction of the spectrograph. Lower panel: collapsed flux profile in the aperture, with the shaded region showing the width of the effective resolution element, which is also given in arc seconds and resolution elements/bins.

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