The morphology and kinematics of the Fine Ring Nebula, planetary nebula Sp 1, and the shaping influence of its binary central star

@article{Jones2011TheMA,
  title={The morphology and kinematics of the Fine Ring Nebula, planetary nebula Sp 1, and the shaping influence of its binary central star},
  author={D. Jones and D. Mitchell and M. Lloyd and D. Pollacco and T. O'Brien and J. Meaburn and N. Observatory and Chalmers Tekniska Hogskola and J. B. C. F. Astrophysics and Queen's University Belfast and Ecole Normale Sup'erieure de Lyon},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2011},
  volume={420},
  pages={2271-2279}
}
  • D. Jones, D. Mitchell, +8 authors Ecole Normale Sup'erieure de Lyon
  • Published 2011
  • Physics
  • Monthly Notices of the Royal Astronomical Society
  • We present the first detailed spatiokinematical analysis and modelling of the planetary nebula Shapley 1 (Sp 1), which is known to contain a close-binary central star system. Close-binary central stars have been identified as a likely source of shaping in planetary nebulae, but with little observational support to date. Deep narrow-band imaging in the light of [O iii] λ5007 A suggests the presence of a large bow shock to the west of the nebula, indicating that it is undergoing the first… CONTINUE READING
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