Fig. 6
The parameters TC and β for a set of internally heated Bonnor-Ebert models with masses of 0.4, 0.8, 1.6, 3.2, and 6.4 M⊙. The solid lines connect models with an internal heating source of given luminosity, 0.0, 0.1, 0.3, 1.0, or 3.0 solar luminosities. The dashed lines connect models of the same mass. The parameters have been derived assuming the source in unresolved.
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