Stars as Artists: The Shaping of Planetary Nebulae

Details Stars as Artists: The Shaping of Planetary Nebulae Stars as Artists: The Shaping of Planetary Nebulae

Nov 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cfa..colle..29b&link_type=abstract

CfA Colloquium Lecture Series Talk

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Scientific paper

Ten years of Hubble images of planetary nebulae have shown their astounding high-order symmetries in the mass that they eject once they start to ascend the AGB. These symmetries are too common, on the one hand, and complex, on the other, to provide any confidence that we presently understand how stars eject mass late in their lives. At the same time trends seen in the Hubble images, their changes with time, and maps of Doppler shifts represent a very nice set of constraints on any proposed mechanism for shaping mass loss. The goal of the talk is to present representative data, identify the interesting patterns that have emerged, and describe broad classes of new types of models which, at this point in the march of science, are guides to organizing our ignorance of how old stars evolve. The most hopeful of these requires the emergence of long-lived magnetic fields released from a spinning core dynamo by very deep convection near the end of the AGB ascent. MHD models are promising, but certainly not yet viable.

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