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

Sara C. Beck; Pei Ying Hsieh; Jean Turner

doi:10.1093/mnras/stab3590

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

Sara C. Beck^*, Pei Ying Hsieh, Jean Turner

^*Corresponding author for this work

School of Physics and Astronomy

Research output: Contribution to journal › Comment/debate

Abstract

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.

Original language	English
Pages (from-to)	2617
Number of pages	1
Journal	Monthly Notices of the Royal Astronomical Society
Volume	510
Issue number	2
DOIs	https://doi.org/10.1093/mnras/stab3590
State	Published - Feb 2022

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abstract = "The authors wish to report an error in the velocity scale of the CO(2- 1) spectra presented in the paper {\textquoteright}SMA Observations of Haro 2: molecular gas around a Hot Superbubble{\textquoteright}. 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{\textquoteright}s main conclusions on the internal kinematics of the galaxy are not affected by this correction.",

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

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