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The polarization of core-collapse supernovae shows that many if not all ofthese explosions must be strongly bi-polar. The most obvious way to producethis axial symmetry is by the imposition of a jet as an intrinsic part of theexplosion process. These jets could arise by MHD processes in the formation ofpulsars and be especially strong in the case of magnetars. The jets will blowiron-peak material out along the axes and other elements from the progenitoralong the equator, a very different composition structure than pictured insimple spherical "onion skin" models. In extreme cases, these processes couldlead to the production of gamma-ray bursts powered by strong Poynting flux.Comment: Contribution to the Fifth Huntsville Conference on Gamma-Ray Bursts,  5 pages, LaTeX, 1 (color) eps figur

The type Ib/c supernova, gamma-ray burst, soft gamma-ray repeater, magnetar connection