The Absence of Extratidal Structure in the Sculptor Dwarf Spheroidal Galaxy
- 1 September 2005
- journal article
- Published by American Astronomical Society in The Astronomical Journal
- Vol. 130 (3) , 1065-1082
- https://doi.org/10.1086/432662
Abstract
The results of a wide-field survey of the Sculptor dwarf spheroidal galaxy are presented. Our aims were to obtain an accurate map of the outer structure of Sculptor, and to determine the level of interaction between this system and the Galaxy. Photometry was obtained in two colours down to the magnitude limits of V=20 and I=19, covering a 3.1 times 3.1 square deg area centred on Sculptor. The resulting colour-magnitude data were used as a mask to select candidate horizontal branch and red giant branch stars for this system. Previous work has shown that the red horizontal branch (HB) stars are more concentrated than the blue HB stars. We have determined the radial distributions of these two populations and show that the overall Sculptor density profile is well described by a two component model based on a combination of these radial distributions. Additionally, spectra of the Ca ii triplet region were obtained for over 700 candidate red giant stars over the 10 square deg region using the 2dF instrument on the Anglo-Australian Telescope. These spectra were used to remove foreground Galactic stars based on radial velocity and Ca ii triplet strength. The final list of Sculptor members contained 148 stars, seven of which are located beyond the nominal tidal radius. Both the photometric and spectroscopic datasets indicate no significant extra-tidal structure. These results support at most a mild level of interaction between this system and the Galaxy, and we have measured an upper mass limit for extra-tidal material to be 2.3 +/- 0.6% of the Sculptor luminous mass. This lack of tidal interaction indicates that previous velocity dispersion measurements (and hence the amount of dark matter detected) in this system are not strongly influenced by the Galactic tidal field.Comment: 53 pages, 23 figures. Accepted for publication in the Astronomical Journal. Some figures are reduced in size, and a full version is available at: ftp://ftp.mso.anu.edu.au/pub/coleman/sculptor.pdKeywords
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This publication has 64 references indexed in Scilit:
- A Two Micron All‐Sky Survey View of the Sagittarius Dwarf Galaxy. IV. Modeling the Sagittarius Tidal TailsThe Astrophysical Journal, 2005
- Population Gradients in Local Group Dwarf Spheroidal GalaxiesThe Astronomical Journal, 2001
- Stellar Population Studies with the SDSS. I. The Vertical Distribution of Stars in the Milky WayThe Astrophysical Journal, 2001
- The First US Naval Observatory CCD Astrograph CatalogThe Astronomical Journal, 2000
- Dwarf spheroidal satellite galaxies without dark matterNew Astronomy, 1997
- Globular Clusters with Tidal Tails: Deep Two-Color Star CountsThe Astronomical Journal, 1995
- The structure of the Sculptor dwarf elliptical galaxy. II - Two-dimensional structureThe Astronomical Journal, 1988
- The structure of the sculptor dwarf elliptical galaxy. I - The radial profileThe Astronomical Journal, 1988
- The structure of the Sculptor systemThe Astronomical Journal, 1980
- A Color-Magnitude Diagram for the Sculptor Dwarf Galaxy.The Astrophysical Journal, 1965