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Fig. 7
H-R diagram for all the spectroscopically confirmed members of ρ Ophiuchi. The models are the NextGen and Dusty isochrones (Baraffe et al. 1998; Chabrier et al. 2000) (upper panel) and the isochrones from Siess et al. (2000) (lower panel) for 1, 5, 10, and 30 Myr, labelled with mass in units of M⊙.
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