Abstract
In Figure 9 of the published article we compared the SkyMapper metallicity distribution functions (MDFs) for the stars in the blue and red sequences with those found by Gallart et al. (2019). The comparison was made with the MDFs available at the time in their preprint submission on arXiv; however, these have since been updated in their final publication. For the sake of consistency we present an updated comparison with the final MDFs by Gallart et al. (2019) in the revised Figure 9. The red MDFs now show better agreement than before, and the blue MDFs still agree very well. (Figure Presented).
| Original language | English |
|---|---|
| Article number | L28 |
| Journal | Astrophysical Journal Letters |
| Volume | 891 |
| Issue number | 1 |
| DOIs |
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| Publication status | Published - 1 Mar 2020 |
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Dive into the research topics of 'Erratum: "Characteristics of the Two Sequences seen in the High-velocity Hertzsprung–Russell diagram in Gaia DR2" (2019, ApJL, 881, L10): DOI: 10.3847/2041-8213/ab321e'. Together they form a unique fingerprint.Cite this
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