Dynamical estimates of the masses of small groups of galaxies

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Catalogs, Digital Simulation, Galactic Mass, Histograms, Hubble Constant, Virial Coefficients

Scientific paper

Numerical simulations of the dynamics of galaxy triplets are conducted
to show the uncertainty of any dynamical estimate of the individual
masses of the triplets. Their strong nonstationarity and the effects of
projection are suggested as the causes. The typical dispersion of the
individual estimates was found to be about 3 orders of magnitude.

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