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Clumping in hot-star winds as function of metallicity: first theoretical predictions and implications for mass-loss diagnostics
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abstract.tex untitled.tex section_Numerical_Simulations_begin_table__.tex begin_table_scalebox_0_75__.tex VH_1_simulation_Jon_Sundqvist__.tex We_use_the_numerical_hydrodynamics__.tex subsection_Line_Strength_We_follow__.tex subsection_Boundary_Conditions_For_each__.tex section_Results__.tex figures/snapshot1/snapshot1.png subsection_Numerical_Results_begin_itemize__.tex figures/isothermal_six_Qbar/isothermal_six_Qbar.png For_our_suite_of_simulations__.tex In_Figure_XX_we_compare__.tex figures/mean_fcl1/mean_fcl1.png We_plot_the_mean_clumping__1.tex section_Discussion_begin_itemize_item__.tex We_used_purely_radial_LDI__.tex