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Periodic activity on the (sub)mm surface of the AGB star Mira A

Andriantsaralaza, M. et al.
arXiv (All) · Papers
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solar-and-stellar-astrophysics
Evolved stars on the asymptotic giant branch (AGB) lose mass through stellar winds launched from their dynamic extended atmospheres. Recent high-angular-resolution observations of the archetypal AGB star Mira A (o Ceti) have revealed compact hotspots on its (sub)millimetre surface, whose origin rema
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