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 ‘bullet’ which appears to be the head of a high velocity jet which causes the entrainment of molecular outflows.
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Hughes, V.A., Cohen, R.J. & Garrington, S. Unravelling cepheus a. Astrophys Space Sci 224, 69–72 (1995). https://doi.org/10.1007/BF00667823
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DOI: https://doi.org/10.1007/BF00667823