RZ Psc, previously seen only as an outflowing UXOR, now shows inverse P Cygni profiles in H-alpha and Ca II 8542, evidence of short-lived magnetospheric accretion episodes.
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Flares of accretion activity of the 20 Myr old UXOR RZ Psc
RZ Psc, previously seen only as an outflowing UXOR, now shows inverse P Cygni profiles in H-alpha and Ca II 8542, evidence of short-lived magnetospheric accretion episodes.