A New Approach to Numerical Modelling of Circumstellar Dust Shells around Pulsating AGB Stars

Details A New Approach to Numerical Modelling of Circumstellar Dust Shells around Pulsating AGB Stars A New Approach to Numerical Modelling of Circumstellar Dust Shells around Pulsating AGB Stars

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..378..277b&link_type=abstract

Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes. ASP Conference Series, Vol. 378, proceedings of the co

Astronomy and Astrophysics

Astronomy

Scientific paper

A time-dependent numerical description of dust-forming circumstellar envelopes around pulsating AGB stars has to account for a variety of very different physical and chemical processes leading to a system of multi--scale, highly non--linear, coupled partial differential equations. We present a new numerical modelling technique for the dust-forming circumstellar envelopes around pulsating AGB stars which allows for independent sophisticated time integration for each spatial grid point and aims at a detailed modelling of relevant processes with very different time scales.

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