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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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For_each_different_bar_Q__.tex
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For_our_suite_of_simulations__.tex
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In_Figure_XX_we_compare__.tex
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VH_1_simulation_Jon_Sundqvist__.tex
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We_plot_the_mean_clumping__.tex
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We_plot_the_mean_clumping__1.tex
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We_use_the_numerical_hydrodynamics__.tex
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We_used_purely_radial_LDI__.tex
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abstract.tex
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begin_table_scalebox_0_75__.tex
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header.tex
layout.md
section_Discussion_begin_itemize_item__.tex
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section_Numerical_Simulations_begin_table__.tex
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section_Results__.tex
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subsection_Boundary_Conditions_For_each__.tex
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subsection_Line_Strength_We_follow__.tex
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subsection_Numerical_Results_begin_itemize__.tex
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title.tex
untitled.tex
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