THE DEVELOPMENT OF SAN LUIS POTOSIIRAL STRUCTURE IN A GALAXY
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UNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
Abstract
The main aim of this paper is to show that by postulating the existence of a rotating and shrinking gaseous bulge with a magnetic field as envisaged, and given a rotation curve, a galaxy will have produced and maintained spiral arms during a reasonably lo