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Cited article:

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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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The red supergiant population in the Perseus arm

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

L. R. Patrick, C. J. Evans, B. Davies, et al.
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