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Emergent surface intensity of a supergiant (*.mpg)
From Numerical simulations of a red supergiant
Bernd Freytag, Centre de Recherche Astronomique de Lyon and Uppsala Astronomical Observatory
Astronomy 10 learning goal M3.2
Computer simulation over several months of the outer layers of a supergiant, such as Betelgeuse, between its main sequence phase, and inevitable type II supernova explosion.
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