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astro-ph.SR 1

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2026 1

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On the Robustness of Bi-Stability Jump Predictions

astro-ph.SR · 2026-06-15 · unverdicted · novelty 4.0

PoWR models at low-to-intermediate Eddington parameters confirm a robust bi-stability jump driven by the Fe IV to Fe III transition, with mass-loss rate increasing by over an order of magnitude and terminal velocity dropping.

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  • On the Robustness of Bi-Stability Jump Predictions astro-ph.SR · 2026-06-15 · unverdicted · none · ref 15

    PoWR models at low-to-intermediate Eddington parameters confirm a robust bi-stability jump driven by the Fe IV to Fe III transition, with mass-loss rate increasing by over an order of magnitude and terminal velocity dropping.