‘Our attention has been drawn to the existence of two papers, Huaman, Carruba & Domingos (2014) and Carruba et al. (2014), which study the dynamics of a few putative V-type candidates in the middle and outer MB, suggested in Carvano et al. (2010). The approach of those papers is limited to the specific study of the dynamical evolution of the objects, without rigorous inspection of the taxonomic properties of their neighbourhood. Consequently, their conclusions are ambiguous and need to be supported by observational data’.
Erratum: Characterization of V-type asteroids orbiting in the middle and outer main belt (Monthly Notices of the Royal Astronomical Society DOI: 10.1093/mnras/stab332)
Lazzarin M.;La Forgia F.
2021
Abstract
‘Our attention has been drawn to the existence of two papers, Huaman, Carruba & Domingos (2014) and Carruba et al. (2014), which study the dynamics of a few putative V-type candidates in the middle and outer MB, suggested in Carvano et al. (2010). The approach of those papers is limited to the specific study of the dynamical evolution of the objects, without rigorous inspection of the taxonomic properties of their neighbourhood. Consequently, their conclusions are ambiguous and need to be supported by observational data’.
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