Dynamical structure of planetary nebulae in three dimensions a numerical solution

Details Dynamical structure of planetary nebulae in three dimensions a numerical solution Dynamical structure of planetary nebulae in three dimensions a numerical solution

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000immm.proc..123g&link_type=abstract

The interstellar medium in M31 and M33. Proceedings 232. WE-Heraeus Seminar, 22-25 May 2000, Bad Honnef, Germany. Edited by El

Physics

Scientific paper

A model of two interacting winds and a nonspherical density function in three dimensions is introduced to study the dynamical structure of planetary nebulae. A fast wind with a mechanical energy interacts with a super wind mass-loss rate of 2 x 10-5 Msun/yr and a velocity of 10 km/s. As a result it produces a dense and luminous medium.

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