This site uses cookies. By continuing to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies policy.

On Kinematic Substructure in the Sextans Dwarf Spheroidal Galaxy*

, , , , , and

Published 2006 April 14 © 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Matthew G. Walker et al 2006 ApJ 642 L41 DOI 10.1086/504522

1538-4357/642/1/L41

Abstract

We present multifiber echelle radial velocity results for 551 stars in the Sextans dwarf spheroidal galaxy and identify 294 stars as probable Sextans members. The projected velocity dispersion profile of the binned data remains flat to a maximum angular radius of 30'. We introduce a nonparametric technique for estimating the projected velocity dispersion surface and use this to search for kinematic substructure. Our data do not confirm previous reports of a kinematically distinct stellar population at the Sextans center. Instead we detect a region near the Sextans core radius that is kinematically colder than the overall Sextans sample with 95% confidence.

Export citation and abstract BibTeX RIS

Footnotes

  • Based on observations using the Magellan telescopes.

Please wait… references are loading.
10.1086/504522