Discovery of s-process Nd in Allende residue

New interpretation is given to the isotopic anomalie detected by Lugmair et al. in an acid-resistant residue of the Allende meteorite. If the the 142Nd excess is due to 146Sm decay, as the discoverers proposed, I argue that the decay has occurred in interstellar grains, so that the concludion that 146Sm(1.03 x 108 yr) was alive in the solar system is premature. I show by renormalizing their data that the discovery is likely to be s-process Nd, confirming the survival of red-giang stardust in carbonaceous interstellar dust