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Cited article:

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Multiplicity among the cool supergiants in the Magellanic Clouds

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Type IIP Supernova Progenitors. III. Blue to Red Supergiant Ratio in Low-metallicity Models with Convective Overshoot

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Betelgeuse Just Is Not That Cool: Effective Temperature Alone Cannot Explain the Recent Dimming of Betelgeuse

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The Period–Luminosity Relations of Red Supergiants in M33 and M31

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Atomic Absorption Line Diagnostics for the Physical Properties of Red Supergiants

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The evolution of massive stars: bridging the gap in the Local Group

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Physical properties of the first spectroscopically confirmed red supergiant stars in the Sculptor Group galaxy NGC 55

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Monthly Notices of the Royal Astronomical Society 468 (1) 492 (2017)