Conference Proceedings

Local Group and Star Cluster Dynamics from HSTPROMO: The Hubble Space Telescope Proper Motion Collaboration

Roeland P van der Marel, Jay Anderson, Andrea Bellini, Gurtina Besla, Paolo Bianchini, Mike Boylan-Kolchin, Julio Chaname, Alis Deason, Do Tuan, Puragra Guhathakurta, Nitya Kallivayalil, Danny Lennon, Davide Massari, Eileen Meyer, Imants Platais, Elena Sabbi, Sangmo Tony Sohn, Mario Soto, Michele Trenti, Laura Watkins Show all

STRUCTURE AND DYNAMICS OF DISK GALAXIES | ASTRONOMICAL SOC PACIFIC | Published : 2014

Abstract

The Hubble Space Telescope (HST) has proven to be uniquely suited for the measurement of proper motions (PMs) of stars and galaxies in the nearby Universe. Here we summarize the main results and ongoing studies of the HSTPROMO collaboration, which over the past decade has executed some two dozen observational and theoretical HST projects on this topic. This is continuing to revolutionize our dynamical understanding of many objects, including: globular clusters; young star clusters; stars and stellar streams in the Milky Way halo; Local Group galaxies, including dwarf satellite galaxies, the Magellanic Clouds, and the Andromeda galaxy; and AGN Black Hole Jets.

University of Melbourne Researchers