MHD Launching and Collimation of PNe and Proto-PNe

Details MHD Launching and Collimation of PNe and Proto-PNe MHD Launching and Collimation of PNe and Proto-PNe

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...201.2201f&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #22.01; Bulletin of the American Astronomical Society, Vol. 34, p.1140

Astronomy and Astrophysics

Astronomy

Scientific paper

In this talk I present new results on magnetohydrodynamic models for planetary and proto-planetary nebulae in which the outflows are driven by a fast magnetic rotator. The rotator may be a star or an accretion disk or both acting in concert. For the case of a disk produced via binary interactions we show that magnetocentrifugally launched winds can power the high momentum outflows associated with Proto-PNe

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