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Dynamical structure of the molecular interstellar medium in an extremely bright, multiply lensed z 3 submillimeter galaxy discovered with Herschel

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Academic year: 2020

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Figure 1. Velocity-integrated CARMA and PdBI maps of CO(J = 3 → 2) and CO(J = 5 → 4) line emission over 777 and 515 km s −1 toward HLSW-01
Figure 3. CO(J = 3 → 2) and CO(J = 5 → 4) line emission contours as shown in Figure 1, but overlaid on 890 μm continuum emission detected with the Submillimeter Array (color scale; 2
Figure 4. CO(J = 5 → 4) line emission contours as shown in Figure 1, but overlaid on 2.2 μm continuum emission (gray scale; smoothed with a 0

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