Dust and windmodelling of born-again PNe cores

Details Dust and windmodelling of born-again PNe cores Dust and windmodelling of born-again PNe cores

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..377l&link_type=abstract

In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A

Physics

Stars: Agb And Post-Agb, Stars: Evolution, Ism: Planetary Nebulae

Scientific paper

It is a long, hard way to a fully consistent evolutionary hydrodynamic model in 3D to describe stellar winds and do we really need it after all?. What makes born-again objects so special in the context of dust and windmodelling? I present a few of my ideas to achieve a hydro code combining photoionization of the gas, dust formation as well as evolution and also radiative transfer in 3D.

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