  We present high-resolution ALMA Band 6 and 7 observations of the tidally
disrupted protoplanetary disks of the RW Aurigae binary. Our observations
reveal the presence of additional tidal streams to the previously observed
tidal arm around RW Aur A. The observed configuration of tidal streams
surrounding RW Aur A and B is incompatible with a single star--disk tidal
encounter, suggesting that the RW Aurigae system has undergone multiple fly-by
interactions. We also resolve the circumstellar disks around RW Aur A and B,
with CO radii of 58 au and 38 au consistent with tidal truncation, and 2.5
times smaller dust emission radii. The disks appear misaligned by 12$^{\circ}$
or 57$^{\circ}$. Using new photometric observations from the American
Association of Variable Star Observers (AAVSO) and All Sky Automated Survey for
SuperNovae (ASAS-SN) archives, we have also identified an additional dimming
event of the primary that began in late 2017 and is currently ongoing. With
over a century of photometric observations, we are beginning to explore the
same spatial scales as ALMA.
