Limits of interacting stellar winds model of planetary nebulae - A numerical study

Details Limits of interacting stellar winds model of planetary nebulae - A numerical study Limits of interacting stellar winds model of planetary nebulae - A numerical study

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...157..101b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 157, no. 1, March 1986, p. 101-112.

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29

Computational Astrophysics, Planetary Nebulae, Plasma Interactions, Stellar Models, Stellar Winds, Conductive Heat Transfer, Radiative Heat Transfer, Stellar Mass Ejection

Scientific paper

The dynamical evolution of planetary nebulae (PNe) was calculated numerically in the scenario of the interacting stellar wind model (ISWM). Radiative losses and heat conduction were included in the calculations together with the SLIC method to follow the surface separating the winds. The general trend of PN evolution is discussed and comparison with some observations are made. Limitations to the validity of ISWM are presented, both based on dynamical and observational grounds. Details of the numerical code are given in the Appendix.

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