SMA Observations of haro 2: molecular gas around a hot superbubble

The authors wish to report an error in the velocity scale of the CO(2-1) spectra presented in the paper ’SMA Observations of Haro 2: molecular gas around a Hot Superbubble’. The error is the result of a bug in the data reduction. The velocities quoted for the CO(2-1) line in this paper are redshifted by ∼25 km s⁻¹  from the correct values. The corrected centroid of the CO(2-1) emission is ∼1445 km s⁻¹, consistent with the HI, and it now appears that the two major CO emission regions probably coincide with clumps 2 and 3 of Méndez & Esteban. The paper’s main conclusions on the internal kinematics of the galaxy are not affected by this correction.

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