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Cited article:

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Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Convection in 3D Simulations of Red Supergiants

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ATOMIUM: Probing the inner wind of evolved O-rich stars with new, highly excited H2O and OH lines

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The inner dust shell of Betelgeuse seen with high-angular-resolution polarimetry

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Spatially Resolved Observations of Betelgeuse at λ7 mm and λ1.3 cm Just prior to the Great Dimming

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The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope

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Pre-supernova evolution, compact-object masses, and explosion properties of stripped binary stars

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Heavy-element Rydberg transition line emission from the post-giant-evolution star HD 101584

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Spatially Resolved Ultraviolet Spectroscopy of the Great Dimming of Betelgeuse

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The Astrophysical Journal 899 (1) 68 (2020)
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Millimeter-wave Point Sources from the 2500 Square Degree SPT-SZ Survey: Catalog and Population Statistics

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Circumstellar CO J = 3→2 detected around the evolving metal-poor ([Fe/H] ≈ −1.15 dex) AGB star RU Vulpeculae

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ALMA and VLA reveal the lukewarm chromospheres of the nearby red supergiants Antares and Betelgeuse

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NOEMA maps the CO J = 2 − 1 environment of the red supergiant $\mu$ Cep★

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The Evolving Radio Photospheres of Long-period Variable Stars

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