Fig. 1.
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Multiband composite images of Haro 11. Top panel: HST WFC3/UVIS observations using the F555W (blue), F665N (green), and F814W (red) filters (Prop. ID 15649, PI. Chandar). Bottom panel: Multiband imaging in Hα emission (HST F665N, Prop. ID 15649; red), Lyα emission (HST ACS/SBC F122M, Prop. ID 9470; green), and the X-ray 3–5 keV band (Chandra ACIS-S, Obs. ID 8175; blue). The HST data are available via MAST at doi:https://doi.org/10.17909/rn22-jy61.
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