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Authors:V A Hughes  R J Cohen  S Garrington
Institution:(1) Astronomy Group, Department of Physics, Queen's University, K7L 3N6 Kingston, Ontario, Canada;(2) Nuffield Radio Astronomy Laboratories, University of Manchester, Jodrell Bank, Macclesfield, SK11 9DL Cheshire, U.K.
Abstract:The monitoring of Cep A over a 13 year period has shown it to contain interesting aspects of star forming regions. In particular, there are two highly time-dependent radio sources which may be evidence for proto-stars losing their magnetic fields, and a lsquobulletrsquo which appears to be the head of a high velocity jet which causes the entrainment of molecular outflows.
Keywords:Star formation  radio sources  molecular outflows  jets
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