What structural feature allows low-mass red dwarfs (below $0.35 M_ ext{odot}$) to consume nearly all of their hydrogen fuel?

Answer

They are fully convective, mixing fuel throughout the entire star

Red dwarfs below the $0.35 M_ ext{odot}$ threshold are fully convective, meaning fresh hydrogen from the outer layers is constantly circulated into the core, allowing them to convert almost all of their hydrogen into fuel.

What structural feature allows low-mass red dwarfs (below $0.35 M_	ext{odot}$) to consume nearly all of their hydrogen fuel?

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