A Spatial Characterization of the Sagittarius Dwarf Galaxy Tidal Tails

Abstract

We measure the spatial density of F turnoff stars in the Sagittarius dwarf tidal stream, from Sloan Digital Sky Survey (SDSS) data, using statistical photometric parallax. We find a set of continuous, consistent parameters that describe the leading Sgr stream's position, direction, and width for 15 stripes in the North Galactic Cap, and 3 stripes in the South Galactic Cap. We produce a catalog of stars that has the density characteristics of the dominant leading Sgr tidal stream that can be compared with simulations. We find that the width of the leading (North) tidal tail is consistent with recent triaxial and axisymmetric halo model simulations. The density along the stream is roughly consistent common disruption models in the North, but possibly not in the South. We explore the possibility that one or more of the dominant Sgr streams has been mis-identified, and that one or more of the `bifurcated' pieces is the real Sgr tidal tail, but we do not reach definite conclusions. If two dwarf progenitors are assumed, fits to the planes of the dominant and `bifurcated' tidal tails favor an association of the Sgr dwarf spheroidal galaxy with the dominant Southern stream and the `bifurcated' stream in the North. In the North Galactic Cap, the best fit Hernquist density profile for the smooth component of the stellar halo is oblate, with a flattening parameter q = 0.53, and a scale length of r_0 = 6.73. The Southern data for both the tidal debris and the smooth component of the stellar halo do not match the model fits to the North, although the stellar halo is still overwhelmingly oblate. Finally, we verify that we can reproduce the parameter fits on the asynchronous Milkyway@home volunteer computing platform.

35 pages, 8 figures, 9 tables. Accepted for publication in The Astrophysical Journal

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Cited by in corpus (12)

• Tracing the tidal streams of the Sagittarius dSph, and halo Milky Way features, with carbon-rich long-period variables
• Stellar Substructures around the Hercules Dwarf Spheroidal Galaxy
• Selecting M-giants with infra-red photometry: Distances, metallicities and the Sagittarius stream
• Structural analysis of the Sextans dwarf spheroidal galaxy
• The Virgo Overdensity Explained
• Extended stellar substructure surrounding the Boötes I dwarf spheroidal galaxy
• Selecting Sagittarius: Identification and Chemical Characterization of the Sagittarius Stream
• Testing the Dark Matter Caustic Theory Against Observations in the Milky Way
• A tangle of stellar streams in the north Galactic cap
• Fitting the density substructure of the stellar halo with MilkyWay@home
• Introduction to Tidal Streams
• MilkyWay@home: Harnessing volunteer computers to constrain dark matter in the Milky Way