Astrophysics and Space Science

, Volume 224, Issue 1–2, pp 69–72 | Cite as

Unravelling cepheus a

  • V. A. Hughes
  • R. J. Cohen
  • S. Garrington
Session A: Protostellar & Pre-Main Sequence Shells and Disks
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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.

Key words

Star formation radio sources molecular outflows jets 

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Copyright information

© Kluwer Academic Publishers 1995

Authors and Affiliations

  • V. A. Hughes
    • 1
  • R. J. Cohen
    • 2
  • S. Garrington
    • 2
  1. 1.Astronomy Group, Department of PhysicsQueen's UniversityKingston, OntarioCanada
  2. 2.Nuffield Radio Astronomy LaboratoriesUniversity of ManchesterCheshireU.K.

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