Figure 6
Location of the three stars in the HR diagram. The solid lines are the theoretical evolutionary models of Blöcker (1995b), labelled with the core mass in solar units. The long-dashed lines show the location of the stars based on the V-band magnitude: from right- to left-hand side He 2-436, Wray 16-423 and StWr 2-21. The square symbols show the specific models of Clegg & Middlemass (1987) used in deriving these lines. The photoionization models are shown by the plus signs: in all cases they are on or to the left-hand side of the corresponding long-dashed line.

Location of the three stars in the HR diagram. The solid lines are the theoretical evolutionary models of Blöcker (1995b), labelled with the core mass in solar units. The long-dashed lines show the location of the stars based on the V-band magnitude: from right- to left-hand side He 2-436, Wray 16-423 and StWr 2-21. The square symbols show the specific models of Clegg & Middlemass (1987) used in deriving these lines. The photoionization models are shown by the plus signs: in all cases they are on or to the left-hand side of the corresponding long-dashed line.

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