Published July 16, 2025
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New line-driven wind mass-loss rates for OB stars with metallicities down to 0.01 Z_o
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1.
Masaryk University
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2.
Czech Academy of Sciences, Astronomical Institute
Description
Fotran77 and Gnuplot codes that calculate hot-star wind mass-loss rate as a function of the stellar parameters.
Reference: Jiri Krticka, Jiri Kubat, Iva Krtickova, New line-driven wind mass-loss rates for OB stars with metallicities down to 0.01 Z_o, 2025, submitted to Astronomy & Astrophysics
Supported by grant GA ČR 25-15910S.
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