Radiative accelerations for evolutionary model calculations
نویسندگان
چکیده
منابع مشابه
Radiative accelerations on Ne in the atmospheres of late B stars
Radiative accelerations on Ne are calculated for the atmospheres of main sequence stars with 11 000 ≤ T eff ≤ 15 000 K. This range corresponds to that of the mercury-manganese (HgMn) stars. The calculations take into account neon fine structure as well as shadowing of neon lines using the entire Kurucz line list, bound-bound, bound-free and free-free opacity of H, He and C as well as some NLTE ...
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