Fig. 5
Comparison of spectroscopic Mspec and evolutionary masses Mevol for the sample stars. Dots mark objects with measured parallaxes (van Leeuwen 2007), circles mark stars where only association distances are available (see Table 2). A few field stars have no reliable parallaxes and are therefore omitted here. Error bars denote 1σ-uncertainties and the dotted line indicates the 1:1 relation.
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