The Local Velocity Field

TL;DR

This paper reviews methods and recent results in mapping the local velocity field of galaxies, highlighting models, data, and future surveys to understand cosmic matter distribution.

Contribution

It provides an overview of modeling techniques and presents new results from a multiattractor model fitted to the SFI++ peculiar velocity data.

Findings

Multiattractor model fits local velocity data well

Future surveys like 2MTF will improve velocity field mapping

Peculiar velocities help infer matter distribution in the universe

Abstract

We only see a small fraction of the matter in the universe, but the rest gives itself away by the impact of its gravity. The distortions from pure Hubble flow (or peculiar velocities) that this matter creates have the potential to be a powerful cosmological tool, but are also a nuisance for extragalactic astronomers who wish to use redshifts to estimate distances to local galaxies. We provide a quick overview of work on the local peculiar velocity field, discussing both simple spherical infall models, non-parametric modeling using redshifts surveys, and full velocity and density field reconstruction from peculiar velocities. We discuss results from a multiattractor model fit to data from the SFI++ sample of peculiar velocities - the best peculiar velocity data currently available. We also talk about the future of samples for the study of the local velocity field, especially the 2MASS Tully-Fisher (2MTF) survey.