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• W2046443312 abstract "We performe N-body simulations of encounters between spherical systems surrounded by a spherical halo. Following a preceding paper with a similar aim, the initial systems include a spherical Jaffe model for the luminous matter and a Hernquist model for the halo. The merger remnants from this sample are mainly slowly rotating, prolate spheroids with a radially anisotropic velocity distribution. The results are compared with real-life ellipticals and with the models without halo in paper I. We argue that elliptical galaxies with evidence of dark matter could be formed in the field via a merger of spheroids surrounded by a dark matter halo, while ellipticals with no evidence of dark matter might be formed via a merger of two spheroids in a cluster." @default.
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• W2046443312 date "2005-08-01" @default.
• W2046443312 modified "2023-09-27" @default.
• W2046443312 title "Encounters between spherical galaxies - II. Systems with a dark halo" @default.
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• W2046443312 doi "https://doi.org/10.1111/j.1365-2966.2005.09243.x" @default.
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