1994/09/29 by Mario Mateo, A. Udalski, M. Szymanski +3 · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1086/117303
13p+3fig; uuencoded comp. postscript
arxiv created 1994/09/29 · openalex publication_date 1995/02/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
We present deep CCD photometry of a field in the newly discovered dwarf spheroidal galaxy in Sagittarius (hereafter Sgr), and of a nearby control field. These data were used to produce color-magnitude (CM) diagrams reaching I ~ 22.3 in both fields. After statistically removing the field stars from the CM diagram we find that Sgr is dominated by a moderately old (age ~10 Gyr) population, significantly younger than a typical globular-cluster population. There is some evidence for a weak intermediate-age component or alternatively a population of blue stragglers. These results confirm that Sgr is a bona fide dwarf spheroidal galaxy, the ninth found orbiting the Milky Way. We have discovered nine short-period variables in the Sgr field, well in excess of the number found in the control field. Seven of these stars have similar apparent magnitudes and are almost certainly RR Lyr stars in Sgr. We have used the minimum-light colors of the RRab variables to determine the reddening of the Sgr field to be E(V-I) = 0.22, or E(B-V) = 0.18 for a normal extinction law. For an assumed RR Lyr luminosity of Mv_ = +0.6 we conclude that the distance of Sgr is 25.2+/-2.8 kpc. The properties of the Sgr giant branch and upper main sequence are consistent with a mean metallicity of [Fe/H]~ -1.1+/-0.3.