Erratum: SMA Observations of haro 2: Molecular gas around a hot superbubble (Monthly Notices of the Royal Astronomical Society DOI: 10.1093/mnras/staa660)

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 M ´endez & Esteban. The paper’s main conclusions on the internal kinematics of the galaxy are not affected by this correction.