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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 3.

Evolution of a stellar polytropic envelope with entropy per baryon S = 45.0 and an initial Bernoulli parameter ε = 0.01 U/μ (corresponding to an initial mass of ≈10 M⊙). Top panel: the Bernoulli parameter, ε, in units of U/μ. Bottom panel: the stellar mass, M, in units of M⊙. Both are presented as a function of time, in units of kiloyears.

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