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Transonic Solutions for Recombination-driven Stellar Winds

  • Authors: Ilan Strusberg, Re'em Sari, Jim Fuller

Ilan Strusberg et al 2026 The Astrophysical Journal Letters 1011 .

  • Provider: AAS Journals

Caption: Figure 6.

The ratio between the radiative luminosity at the critical point and the mass-loss rate (given by Equation (19)) times the Bernoulli parameter, as a function of entropy (in units of kB) and the Bernoulli parameter ε (in units of U/μ), for Bernoulli parameter values between 0.01 and 0.99. The red zone in the upper-left corner is where radiative diffusion becomes dominant.

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