BB303

Proper motion of Galaxies in and beyond the Local Group

Abstract

In the concordance Lambda-CDM cosmological model, galaxies grow hierarchical in mass by accreting smaller galaxies. Nearby examples of this cosmic cannibalism are found in the environments of the Milky Way and the Andromeda Galaxy (M31), in the Local Group (LG), nearby galaxy groups, and clusters. However, a description of galaxy interactions cannot be complete without knowing the full 3d space motions of the galaxies. Exploiting the sensitivity upgrade of the major VLBI facilities opens up the possibility to do more targets than previously possible. The main goal of this project is to measure accurate *absolute* space motions of galaxies in the LG, in the M81 group of galaxies, and even inside the Virgo Cluster. This will lead, together with detailed simulations to a better understanding of matter distribution in- and outside the LG, and the evolution of galaxies in these environments . The LG is also a good test bed for alternative theories of gravity (e.g. MOND). Furthermore, geomet

Investigators

Name Institution
GBT Operator Green Bank Observatory
vlbaops vlbaops National Radio Astronomy Observatory
Jacqueline van Gorkom Columbia University
Andrea Tarchi Istituto Nazionale di Astrofisica
Lorant Sjouwerman National Radio Astronomy Observatory
E. Roediger Bremen, Jacobs University
Tom Oosterloo Netherlands Institute for Radio Astronomy
Laurent Loinard México, Universidad Nacional Autónoma de; Harvard University
Avi Loeb Center for Astrophysics | Harvard & Smithsonian
Chris Henkel Max-Planck-Institut für Radioastronomie
Mike Garrett Manchester, University of
Heino Falcke Netherlands Institute for Radio Astronomy; Nijmegen, Radboud Universiteit
Jeremy Darling Colorado at Boulder, University of
Geoff Bower California at Berkeley, University of
Karl Menten Max-Planck-Institut für Radioastronomie
Mark Reid Center for Astrophysics | Harvard & Smithsonian
Andreas Brunthaler * Max-Planck-Institut für Radioastronomie
effobs effobs Max-Planck-Institut für Radioastronomie
vlbiobs vlbiobs National Radio Astronomy Observatory

* indicates the PI