Solving For The Dynamic Masses Of Galaxies With NAM.

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We describe a technique to search in mass-space for the combination of masses of galaxies and groups out to the Virgo Cluster distance that results in model peculiar velocities from Numerical (Least) Action Methods that are in best correspondence with the observed redshifts. We now have accurate TRGB and Cepheid distances for many galaxies in this local volume, therefore accurate models of the flow history of galaxies can be calculated. We use present location and the assumption of low peculiar velocities at early times to derive orbits and thus present velocities. The problem is unconstrained because the individual masses of galaxies are unknown, but a downhill simplex minimization through mass-space with a Chi^2 based on redshifts estimate these total masses. The total masses are, of course, mostly comprised of dark matter.

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