Shaping of Planetary Nebulae by Magnetic Fields

Details Shaping of Planetary Nebulae by Magnetic Fields Shaping of Planetary Nebulae by Magnetic Fields

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008pasp..120.1267p&link_type=abstract

The Publications of the Astronomical Society of the Pacific, Volume 120, Issue 874, pp. 1267-1270.

Astronomy and Astrophysics

Astronomy

2

Ism

Scientific paper

Superwind production triggered by internal MHD effects in Red Giants is considered. Huge vortices of gas are predicted in and above the atmosphere during the peaked phase of ejection. Examination of the results clearly indicates a strong departure from the idealized spherical photosphere for these objects. Incidence on nonsphericity commonly observed in many planetary nebulae is discussed.

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