Multi-epoch SPHERE observations of the AB Aurigae disk show sub-Keplerian rotation inside ~60 au and Halpha emission from feature f1 consistent with accretion onto a several-Jupiter-mass protoplanet candidate.
The latter is the relevant for estimating the accretion luminosity and the mass ac- cretion rate
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Destructuring the disk of AB Aurigae: Dynamics and accretion
Multi-epoch SPHERE observations of the AB Aurigae disk show sub-Keplerian rotation inside ~60 au and Halpha emission from feature f1 consistent with accretion onto a several-Jupiter-mass protoplanet candidate.