Fig. 2
Radial Mach number of the gas for a stellar mass of 1.0 M⊙. The Mach number is defined as a quotient of radial velocity and the sound speed Ma = | ur | /cs. The different colours correspond to the different stellar rotation rates ω = Ω∗/ΩK(R∗). The smaller box inside the graph is a zoom in of the inner edge; the light grey frame denotes the zoom area.
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