Figure 6
Histogram of derived radial velocities of FLAMES targets. The dashed curves are Gaussians fit to the Sgr dSph and Galactic populations, as described in Section 3.3. The Galactic population is relatively well separated, lying almost exclusively below 100 km sāˆ’1 (vertical line).

Histogram of derived radial velocities of FLAMES targets. The dashed curves are Gaussians fit to the Sgr dSph and Galactic populations, as described in Section 3.3. The Galactic population is relatively well separated, lying almost exclusively below 100 km sāˆ’1 (vertical line).

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