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Table 2

Properties for the locally isothermal disk models without a planet.

Name Characterization Section

Model 1 standard model 2.1
Model 2 closed inner boundary 3.2
Model 3 different inner radii 3.3

Notes. Model 1 is our reference model that is described in detail in Sect. 2.1. In the other two models certain (numerical) parameter variations that have been applied in order to compare to previous models, in particular by Pierens & Nelson (2013). They are described in the quoted sections.

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