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A prevalence of dynamo-generated magnetic fields in the cores of intermediate-mass stars
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After_some_time_intermediate_mass__.tex
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Considering_again_the_low_mass__.tex
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Figure_1_shows_the_oscillation__.tex
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Figure_3_shows_that_the__.tex
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In_Fig_2_we_show__.tex
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In_Fig_4_we_show__.tex
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Our_results_show_that_main__.tex
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The_high_occurrence_rate_of__.tex
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The_stars_in_Fig_2__.tex
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Turning_to_higher_masses_we__.tex
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We_measured_the_amount_of__.tex
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We_quantify_the_mass_dependence__.tex
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abstract.tex
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authors.tex
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header.tex
layout.md
section_Acknowledgments_This_paper_was__.tex
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section_Main_Red_giants_are__.tex
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section_Methods_subsection_Dipole_mode__.tex
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title.tex
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