Absolute Proper Motion of the Sagittarius Dwarf Galaxy and of the Outer Regions of the Milky Way Bulge

  • Dinescu D
  • Girard T
  • van Altena W
  • et al.
46Citations
Citations of this article
6Readers
Mendeley users who have this article in their library.

Abstract

We have determined the absolute proper motion of the Sagittarius dwarf spheroidal galaxy (Sgr) from the Southern Proper Motion Catalog 3, by selecting red giant candidates from the Two Micron All Sky Survey. We obtain μlcosb=-2.35+/-0.20 and μb=2.07+/-0.20 mas yr-1. Using the same procedure, we also determine the absolute proper motion of the bulge in the region of the sky that overlaps with Sgr. For the bulge, we obtain μlcosb=-5.86+/-0.14 and μb=-0.59+/-0.14 mas yr-1, at l=7.6d and b=-21.2d. The absolute proper motions are on the International Celestial Reference System via Hipparcos Catalog stars.

Cite

CITATION STYLE

APA

Dinescu, D. I., Girard, T. M., van Altena, W. F., & López, C. E. (2005). Absolute Proper Motion of the Sagittarius Dwarf Galaxy and of the Outer Regions of the Milky Way Bulge. The Astrophysical Journal, 618(1), L25–L28. https://doi.org/10.1086/427731

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free