Planetary Nebulae with Double Shells and Haloes: Insights from Hydrodynamical Simulations

Details Planetary Nebulae with Double Shells and Haloes: Insights from Hydrodynamical Simulations Planetary Nebulae with Double Shells and Haloes: Insights from Hydrodynamical Simulations

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002rmxac..12..144s&link_type=abstract

Ionized Gaseous Nebulae, a Conference to Celebrate the 60th Birthdays of Silvia Torres-Peimbert and Manuel Peimbert, Mexico City

Astronomy and Astrophysics

Astronomy

5

Hydrodynamics, Planetary Nebulae: General, Stars: Agb And Post-Agb, Stars: Mass Loss, Stars: Winds, Outflows

Scientific paper

We combined hydrodynamical simulations with stellar evolutionary
calculations based on prescribed mass-loss rates in order to get a
better understanding of how structure and kinematics of circumstellar
matter develop with time during the late AGB and the following post-AGB
and Planetary Nebula (PN) evolution.

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