Proper motion of the Sagittarius dwarf galaxy based on Hubble space telescope imaging

Carlton Pryor, Slawomir Piatek, Edward W. Olszewski

Research output: Contribution to journalArticlepeer-review

28 Scopus citations

Abstract

We have derived a proper motion of Sagittarius using archival data obtained with the Hubble Space Telescope. The data consist of imaging at three epochs with a time baseline of about four years in three distinct fields. The zero point for the proper motion is based on the foreground Galactic stellar populations along the line of sight. The measured proper motion in the Galactic coordinate system is (μ, μb) = (-2.615 ± 0.22, 1.87 ± 0.19) mas yr-1 and in the equatorial coordinate system is (μα, μδ) = (-2.75 ± 0.20, - 1.65 ± 0.22) mas yr-1. Removing the contribution of the motion of the Sun and of the LSR to the measured proper motion produces a Galactic rest-frame proper motion of (μGrf , μGrf b) = (-0.82 ± 0.22, 1.98 0.19) mas yr -1 and (μGrf α, μGrf δ) = (-2.14 ± 0.20, 0.03 ± 0.20) mas yr -1. The implied space velocity with respect to the Galactic center is (Π, Θ, Z) = (141.9 ± 6.9, 117 ± 29, 238 ± 27) km s-1. This velocity implies that the instantaneous orbital inclination is 67°, with a 95% confidence interval of (58°, 79°). We also present photometry and membership probabilities for the stars in our sample, which can be used to generate color-magnitude diagrams for stellar populations selected by proper motion.

Original languageEnglish (US)
Pages (from-to)839-856
Number of pages18
JournalAstronomical Journal
Volume139
Issue number3
DOIs
StatePublished - 2010

Keywords

  • Astrometry
  • Galaxies: dwarf
  • Galaxies: individual (Sagittarius)

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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