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

The 2D gasdynamical simulations of gas 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 calculati...

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Bibliographic Details
Main Author:	E. Yu. Kilpio
Format:	Article
Language:	English
Published:	Odessa I. I. Mechnykov National University 2017-04-01
Series:	Odessa Astronomical Publications
Online Access:	http://oap.onu.edu.ua/article/view/99459

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