  Observations have shown the existence of narrow, very long, straight jets
emitted by some newly forming stars (1). It is highly likely that stars forming
in the plane of a spiral galaxy do so in the presence of an almost uniform
magnetic field. In the Strong Magnetic Field model (SMF), gravitational
collapse of a highly conducting plasma in the presence of such a field will
result in the formation of a stable, highly relativistic current loop (storage
ring) around the central object. The concept was first described by Greyber
(2-14). In the figures in Mestel & Strittmatter (15), one can see such a
storage ring beginning to form. Such an increasing dipole magnetic field
(formed temporarily for 10$^4$ to 10$^6$ years) will produce, accelerate and
confine a narrow, very long, straight jet. When the density becomes too high,
either the loop is destroyed, or the current-carrying plasma ring is buried
inside the newly forming star and is the source of primordial stellar
magnetism.
