What can Gaia proper motions tell us about Milky Way dwarf galaxies?

S. Jin, A. Helmi, M. Breddels

Research output: Chapter in Book/Report/Conference proceedingConference contributionAcademic

Abstract

We present a proper-motion study on models of the dwarf spheroidal galaxy Sculptor, based on the predicted proper-motion accuracy of Gaia measurements. Gaia will measure proper motions of several hundreds of stars for a Sculptor-like system. Even with an uncertainty on the proper motion of order 1.5 times the size of an individual proper-motion value of ˜10 mas/century, we find that it is possible to recover Sculptor's systemic proper motion at its distance of 79 kpc.
Original languageEnglish
Title of host publicationThe Milky Way Unravelled by Gaia
Subtitle of host publicationGREAT Science from the Gaia Data Releases
PublisherEAS Publications Series
Pages241-245
Volume67-68
DOIs
Publication statusPublished - Jul-2014

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