Higher-metallicity massive stars show larger accretion-driven luminosity increases despite being more extended, and flip to a cool inflated state at lower accretion rates than low-metallicity stars.
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High Power Accretion in Massive Binary Systems and the Impact of Metallicity
Higher-metallicity massive stars show larger accretion-driven luminosity increases despite being more extended, and flip to a cool inflated state at lower accretion rates than low-metallicity stars.