Heavy elements originate from various stellar processes, not solely from supernovae. The slow (s) process occurs in red giants, while the rapid (r) process is associated with supernovae, although much of the material produced may fall back into the neutron star. Supernovae can produce iron, but the specific isotopic composition indicates that some iron remains with the star. White dwarf stars can also undergo supernovae without fusing iron, primarily through carbon fusion. Overall, not all stars that explode as supernovae necessarily have iron present in their composition.