What causes the large extensions of red supergiant atmospheres? Comparisons of interferometric observations with 1D hydrostatic, 3D convection, and 1D pulsating model atmospheres

B. Arroyo-Torres*, M. Wittkowski, A. Chiavassa, M. Scholz, B. Freytag, J. M. Marcaide, P. H. Hauschildt, P. R. Wood, F. J. Abellan

*Corresponding author for this work

    Research output: Contribution to journal › Article › peer-review

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