Winds from 100 old AGB stars in M31's nuclear star cluster can explain the observed low accretion rate and X-ray luminosity of M31*.
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Wind-fed Supermassive Black Hole Accretion by the Nuclear Star Cluster: the Case of M31*
Winds from 100 old AGB stars in M31's nuclear star cluster can explain the observed low accretion rate and X-ray luminosity of M31*.