摘要：In Sect. 2.5, we did not take into account the CO(2−1)/CO(1−0)
ratio to derive the mass of the clumps observed by ALMA. This
corresponds to an error of a factor of about two, compared with
thatobtainedwhenusingtheratioof0.55givenbyCharmandaris
et al. (2000). With such a factor, the total molecular gas mass of
the clumps is M H S ∼ 1.6 × 10 5 M ? . We provide a new version of
Table 2, which shows the corrected values of the molecular gas
mass for the clumps.
关键词：methods: data analysis;galaxies: individual: Centaurus A;galaxies: evolution;galaxies: interactions;galaxies: star formation;errata, addenda
