Statistics – Computation
Scientific paper
Jun 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kfnt....4...44g&link_type=abstract
Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 4, May-June 1988, p. 44-54. In Russian.
Statistics
Computation
Galactic Nuclei, Gas Dynamics, Interstellar Gas, Shock Waves, Stellar Winds, Active Galactic Nuclei, Computational Astrophysics, Stellar Envelopes
Scientific paper
Using NGC 5128 as an example, it is shown that, with acceptable parameter values, the shock-wind mechanism can provide the dynamics of the interstellar gas swept up by a galactic wind from an active nucleus necessary for shell-like structures to form. The periodically repeating star formation process in the gas shell due to the interaction between galactic wind and the interstellar medium and the recurrent activity of the nucleus lead to the formation of the star shell system observed in NGC 5128.
Gnatyk B. I.
Krol' V. A.
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