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A prevalence of dynamo-generated magnetic fields in the cores of intermediate-mass stars
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abstract.tex section_Main_Red_giants_are__.tex figures/example_spectra3/example_spectra.png Figure_1_shows_the_oscillation__.tex We_measured_the_amount_of__.tex In_Fig_2_we_show__.tex The_stars_in_Fig_2__.tex We_quantify_the_mass_dependence__.tex Figure_3_shows_that_the__.tex figures/vis_vs_numax2/vis_vs_numax2.png figures/histogram/tmp.PNG In_Fig_4_we_show__.tex Considering_again_the_low_mass__.tex Turning_to_higher_masses_we__.tex The_high_occurrence_rate_of__.tex Our_results_show_that_main__.tex After_some_time_intermediate_mass__.tex figures/b_crit_nu_mass1/b_crit_nu_mass_6_6.png section_Methods_subsection_Dipole_mode__.tex section_Acknowledgments_This_paper_was__.tex