• Sub-surface convection zones in hot massive stars and their observable consequences

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	bibliography		delete
	figures		delete
	A Physical Origin of Microturbulence.tex		delete
	Abstract.tex		delete
	Acknowledgements.tex		delete
	Again_multidimensional_hydrodynamic_simulations.tex		delete
	As_a_consequence_even.tex		delete
	As_outlined_above.tex		delete
	As_pointed_out_by.tex		delete
	Buoyant Rise.tex		delete
	Clumping and Subsurface Convection.tex		delete
	Clumping in O Stars.tex		delete
	Clumping in WR.tex		delete
	Clumps Size.tex		delete
	Comparing_Figrefpulsationplot_with_the.tex		delete
	Connection With Surface Phenomena.tex		delete
	Connections to Observations.tex		delete
	Development of Convection.tex		delete
	Eq: Acoustic Waves Flux.tex		delete
	Eq: Average.tex		delete
	Eq: Diffusion Convection.tex		delete
	Eq: Diffusion Equation.tex		delete
	Eq: Energy Ratio.tex		delete
	Eq: Equipartition.tex		delete
	Eq: Ficks Law.tex		delete
	Eq: Gravity Waves Flux.tex		delete
	Eq: Ledoux Criterion.tex		delete
	Eq: Rayleigh Criterion.tex		delete
	Eq: Velocity.tex		delete
	Estimate Clumps Number.tex		delete
	Figurerefhrdvel_shows_the_isocontours.tex		delete
	Finally_we_note_that.tex		delete
	From_Figuresref20zsunsurf_andref60zsunsurf_three.tex		delete
	Grid.tex		delete
	Helium Convection Zone.tex		delete
	Hot_luminous_stars_show.tex		delete
	In_Figrefmicrolmc_we_show.tex		delete
	In_Sectrefmagnetic_we_proposed.tex		delete
	In_order_to_compare.tex		delete
	In_the_following_we.tex		delete
	Introduction.tex		delete
	Line Driven Instability.tex		delete
	Line Profile Variability.tex		delete
	MLT.tex		delete
	Mass Discrepancy.tex		delete
	Microturbulence.tex		delete
	More Implications.tex		delete
	Nonradial Pulsations.tex		delete
	Observationally_the_classical_betaCephei.tex		delete
	Photospheric_microturbulence_is_routinely.tex		delete
	Pulsation and Microturbulence.tex		delete
	Results.tex		delete
	Rotation_may_play_an.tex		delete
	Several_classes_of_OBstar.tex		delete
	Significant Correlation.tex		delete
	Subsurface Convection in Hot Massive Stars.pdf		delete
	Subsurface Convection in Hot Massive Stars.tex		delete
	Surface Magnetic Fields.tex		delete
	The_BruntVaisala_frequency_in.tex		delete
	The_FeCZ_could_also.tex		delete
	The_convective_cells_in.tex		delete
	The_microturbulent_velocity.tex		delete
	The_radial_extent_of.tex		delete
	While_in_the_discussed.tex		delete
	Wind Clumping.tex		delete
	Winds and Composition.tex		delete
	abstract.tex		delete
	clumps.tex		delete
	equation_Deltalambda_D__fraclambdacsqrtfrac2_mathcalR.tex		delete
	header.tex
	itemize_item_For_given_luminosity.tex		delete
	layout.md
	method.tex		delete
	resulting_in_maximum_emission.tex		delete
	sectionComparison_with_observationslabelcomparison.tex		delete
	sectionConcluding_remarks.tex		delete
	subsectionMagnetic_fieldslabelmagnetic.tex		delete
	subsectionMicroturbulencelabelmicro.tex		delete
	subsectionRotating_modelslabelrotation_We_considered.tex		delete
	title.tex