2D Modelling of the Gas Flow Structure in the Symbiotic Star Z Andromedae

Details 2D Modelling of the Gas Flow Structure in the Symbiotic Star Z Andromedae 2D Modelling of the Gas Flow Structure in the Symbiotic Star Z Andromedae

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001oap....14...41k&link_type=abstract

Odessa Astronomical Publications, 14, 41-43

Astronomy and Astrophysics

Astronomy

1

Stars: Binary: Symbiotic, Stars: Gas Flow, Stars: Individual: Z And

Scientific paper

The 2D gasdynamical simulations of gas flow structure in the symbiotic star Z And have been carried out for different stellar wind regimes. Since the mechanisms of gas acceleration in stellar atmospheres are not well studied, the parametric representation of gas accelerating force was used. The calculations for various stellar wind velocity regimes have shown that for realistic cases the accretion discs in the system were formed.

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