Fig. 2.
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Velocity distribution of molecular and ionized gas, as well as the stellar components, in Haro 11. Top: Systemic-velocity-subtracted intensity-weighted velocity field (moment 1, 4 × rms) of CO(1–0) emission line. Middle: systemic velocity-subtracted intensity-weighted velocity field of Hα emission. Bottom: Stellar velocity map derived from the SSP fitting results. Black contours and red contours represent the intensities of CO(1–0) and Hα emission lines, respectively.
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