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- W3123024736 abstract "A kinematical analysis applied to a sample of galaxy clusters indicates that the differences between the velocity distributions of elliptical and spiral galaxies are associated with the shape of their orbit families. The orbital anisotropies present in each morphological population could be measured with a parameter that is the ratio of the radial and tangential velocity dispersions, which can be recovered through the observed line-of-sight velocity distribution. When a Gaussian velocity distribution is assumed, having different dispersions along the radial and tangential directions, we conclude that the orbits of elliptical galaxies in clusters are close to radial, while spirals have more circularly shaped or isotropic orbits. Lenticulars galaxies share an intermediate orbital parameter, between spirals and ellipticals." @default.
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- W3123024736 date "1998-04-01" @default.
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- W3123024736 title "Shape of the Galactic Orbits in Clusters" @default.
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- W3123024736 doi "https://doi.org/10.1086/305395" @default.
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