Existing measurements of the parallax or distance modulus for the Pleiades cluster or individual cluster members, all expressed in parsecs. Figure adapted from Melis et al. (2014). The point indicated with “VLBI” is the distance corresponding to the parallax determined by Melis et al. (2014), while the point indicated with “Spectroscopic twins” is the distance corresponding to the parallax determined by Mädler et al. (2016). The references for the rest of the points can be found in Melis et al. (2014).
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