Statistics – Computation
Scientific paper
Jul 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kyome..51..198m&link_type=abstract
Kyoto University, Faculty of Engineering, Memoirs (ISSN 0023-6063), vol. 51, July 1989, p. 198-205. Research supported by the Ya
Statistics
Computation
3
Axisymmetric Flow, Computational Astrophysics, Computational Fluid Dynamics, Computerized Simulation, Gravitational Effects, Stellar Winds, Hypersonic Flow, Stellar Mass Accretion, Supersonic Flow, Upstream, Video Tapes
Scientific paper
Numerical simulations of axisymmetric flow in four different astrophysical situations are performed, and their results are visualized by using a video movie. The situations considered are (1) an accretion flow on to a gravitating compact object allowing maximum accretion; (2) a jet formation in a flow past a gravitating rigid sphere; (3) an interaction between a supersonic wind from a central object and a uniform supersonic incident flow; and (4) a wind bubble formed by spherical supersonic wind.
Fujimoto Yuzo
Koide Hiroshi
Matsuda Takuya
Sawada Keisuke
Sekino Nobuhiro
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