New empirical mass-loss recipe for UV radiation line-driven winds of hot stars across various metallicities

Open Access

Fig. 6

HRD containing the positions of the stars in our sample for the Galaxy (left), LMC (middle), and SMC (right) over-plotted by stellar evolution tracks using our mass-loss recipe (solid lines) and the standard wind mass-loss rates (dashed lines) and an initial rotation velocity of v_{rot, ini} = 100 km s⁻¹. The individual stars are color-coded by their current mass.

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