Correction: The distribution and morphologies of Fornax Cluster dwarf galaxies suggest they lack dark matter (Monthly Notices of the Royal Astronomical Society (2022) 515:2 (2981–3013) DOI: 10.1093/mnras/stac1765)

Elena Asencio*, Indranil Banik*, Steffen Mieske, Aku Venhola, Pavel Kroupa, Hongsheng Zhao

*Corresponding author for this work

Research output: Contribution to journalComment/debatepeer-review

Abstract

This is an erratum to the paper ‘The distribution and morphologies of Fornax Cluster dwarf galaxies suggest they lack dark matter’, published in MNRAS, 515 (2), 2981−3013 (2022). The caption of its fig. 1 is incorrect with regards to the morphological classifications of the dwarfs shown in the first and third rows of the figure. The dwarf in the first row is actually ‘undisturbed’, while the dwarf in the third row is ‘very disturbed’. The dwarf in the middle row is ‘mildly disturbed’, as stated in the original paper. For clarity, we have reproduced this figure with the corrected caption. As these were purely typographical errors and the correct morphological classifications were used in the subsequent analysis, the rest of the original publication is completely unaffected.

Original languageEnglish
Pages (from-to)2718
Number of pages1
JournalMonthly Notices of the Royal Astronomical Society
Volume522
Issue number2
DOIs
Publication statusPublished - 1 Jun 2023

Keywords

  • addenda-gravitation-galaxies
  • clusters
  • dwarf-galaxies
  • errata
  • Fornax-galaxies
  • individual
  • interactions-galaxies
  • statistics-dark matter

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