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The Magnetic Fields in the Envelopes of Proto-Planetary Nebulae

Published online by Cambridge University Press:  07 August 2017

J.Y. Hu
J.Y. Hu*
Affiliation:
Beijing Observatory, Academia Sinica, Beijing, 100080, China

Extract

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It is possible that the magnetic field plays important role in the formation of planetary nebulae(Poscoli, 1992). In order to measure the strength of magnetic field in the envelope of protoplanetary nebulae(PPNe) we have used the Max-Planck-Institut fur Radioastronomie 100-m telescope at Effelsberg to obtain the high frequency resolution and high signal-to-noise ratio 1612 MHz spectra of PPNe, IRAS08005-2356, 18276-1431, and 20406+2953 in both circular polarization. The nature of PPN of these objects are confirmed by Slikhuis et al.(1991), Le Bertre(1987), and Hu et al.(1992) based on the extensive optical, infrared and radio molecular line observations.

Type
IV. Planetary Nebulae Connection: Evolution from the AGB
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 381
Copyright
Copyright © Kluwer 1993 

References

Hu, J. Y. et al.,1992, in preparing.Google Scholar
Le Bertre, T., 1987, A&A, 180,160.Google Scholar
Pascoli, G.,1992, PASP,104, 350.CrossRefGoogle Scholar
Slijkhuis, S. et al.,1991, A&A,248, 547.Google Scholar
Zell, P. J., Fix, J. D.,1991, ApJ,369,506.CrossRefGoogle Scholar