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- W2155973872 abstract "The observed infall of galaxies into the Virgo cluster puts strong constraints on the mass of the cluster. A non-parametric fully non-linear description of the infall can be made with orbit reconstructions based on Numerical Action Methods. The mass of the cluster is determined to be km/s.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html" @default.
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- W2155973872 date "2004-03-01" @default.
- W2155973872 modified "2023-09-27" @default.
- W2155973872 title "Action model of infall into the Virgo cluster" @default.
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- W2155973872 doi "https://doi.org/10.1017/s1743921304000432" @default.
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