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Magnetic fields in PNe and other evolved low-mass and intermediate-mass stars

  • Laurence Sabin (a1), Qizhou Zhang (a2), Gregg A. Wade (a3), Agnès Lèbre (a4) and Roberto Vázquez (a1)...

Magnetic fields are likely to be an efficient mechanism which can affect evolved intermediate mass stars (i.e. post-AGB stars and planetary nebulae) in different ways such as via the shaping of their envelope. However, observational probes for the presence of those fields are still scarce. I will present a summary of the works, including those from our group, on the detection and measurement of magnetic fields in various evolved objects.

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Proceedings of the International Astronomical Union
  • ISSN: 1743-9213
  • EISSN: 1743-9221
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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