Kinematics & Chemistry of Halo Substructures: The Vicinity of the Virgo Over-Density

Abstract

We present observations obtained with the AAT's 2dF wide field spectrograph AAOmega of K-type stars located within a region of the sky which contains the Virgo Over-Density and the leading arm of the Sagittarius Stream. On the basis of the resulting velocity histogram we isolate halo substructures in these overlapping regions including Sagittarius and previously discovered Virgo groups. Through comparisons with N-body models of the Galaxy-Sagittarius interaction, we find a tri-axial dark matter halo is favoured and we exclude a prolate shape. This result is contradictory with other observations along the Sagittarius leading arm, which typically favour prolate models. We have also uncovered K-giant members of Sagittarius that are notably more metal poor ([Fe/H] = -1.7 +/- 0.3 dex) than previous studies. This suggests a significantly wider metallicity distribution exists in the Sagittarius Stream than formerly considered. We also present data on five carbon stars which were discovered in our sample.

accepted to AJ

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Cited by in corpus (16)

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• The Virgo Overdensity Explained
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• The 300km/s stellar stream near Segue 1: Insights From high-resolution spectroscopy of its brightest star
• Forward and Back: Kinematics of the Palomar 5 Tidal Tails