4 November 2004
4 November 2004
Speaker: Bruce Balick (University of Washington)
Title:
Stars as Artists: The Shaping of Planetary Nebulae
Abstract:
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.
Video of the Presentation
(Talks can be viewed with RealPlayer. Free download
is available from
www.real.com
)
References for students:
-
The extraordinary deaths of ordinary stars, B. Balick and A. Frank,
Scientific American, vol. 296, p26, July 2004
-
Sowing the seeds of asymmetry, R. Sahai, in Asymmetrical Planetary
Nebulae III, ASP Conference Series Vol 313, p141, 2004
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