Erratum: ALMA Detects CO(3-2) within a Super Star Cluster in NGC 5253 (Astrophysical Journal (2017) 846 73 DOI: 10.3847/1538-4357/aa8669)

Jean L. Turner*, S. Michelle Consiglio, Sara C. Beck, W. M. Goss, Paul T.P. Ho, David S. Meier, Sergiy Silich, Jun Hui Zhao

*Corresponding author for this work

Research output: Contribution to journalComment/debate

Abstract

The authors wish to report an error in the R.A. given for Cloud D1 in Table 1 of the published article. As stated in the text, Cloud D1 is coincident to within a fraction of the 0 3 beam with the supernebula (Turner & Beck 2004). It is not coincident with visible clusters (Calzetti et al. 2015; Smith et al. 2016) as reported by Cohen et al. (2018). A corrected Table 1 is presented here, with the corrected R.A.. Since the error was typographical in nature, there are no other changes to the published article or conclusions, or to subsequent papers (Consiglio et al. 2017; Cohen et al. 2018) using these data. The authors thank Linda Smith and the participants of the 2019 Guillermo Haro Workshop for revealing this error. (Table Presented).

Original languageEnglish
Article number185
JournalAstrophysical Journal
Volume882
Issue number2
DOIs
StatePublished - 10 Sep 2019

Funding

FundersFunder number
Academia Sinica
National Radio Astronomy Observatory
UCLA Department of Physics
Tel Aviv University

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