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- W79902275 abstract "The non-dissipative evolution of an aspherical initially small density perturbation and the collapse of the resulting bound object (protogalaxy) is studied numerically by the n-body method. The investigation is based on an improved version of the model proposed by Voglis N. and Hiotelis N. (1989, Astron. Astrophys., 218). This model is based on Aasheth's n-body code and takes into account the dynamical effects on the evolution of the protogalaxy of both the close neighbouring material and the extensive mass environment" @default.
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- W79902275 date "1991-09-01" @default.
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- W79902275 title "Dissipationless galaxy formation from non-isolated density perturbations" @default.
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