  We present a new abundance analysis of the super Li-rich star J37 and a
comparison star in NGC 6633. We confirm the result of Deliyannis et al. that
J37 has a Li abundance well above the meteoritic value, and we also confirm
that Al, S, Si, Ca, Fe and Ni are super-solar, and C is sub-solar. We
additionally find that Na, Sc, Ti are super-solar, while O is sub-solar. The
abundance pattern of metals in J37 is generally consistent with the bulk
composition of the Earth. We propose that accretion of circumstellar matter is
the best explanation for these abundance anomalies, although we cannot rule out
a secondary contribution from diffusion.
