Internal kinematics of the Andromeda II dwarf spheroidal galaxy

The High-Resolution Echelle Spectrometer on the Keck I telescope has been used to measure nine radial velocities having a median precision of similar or equal to 2 km s(-1) for seven red giants belonging to the isolated dwarf spheroidal galaxy Andromeda II (And IT). We find a weighted mean radial velocity of (v) over bar(r), = -188 +/- 3 km s(-1) and a central velocity dispersion of sigma(0) = 9.3(-2.6)(+2.7) km s(-1). There may be evidence for a radial velocity gradient across the face of the galaxy, although the significance of this result is low because of the small number of stars having measured velocities. Our best estimate for the global mass-to-light ratio of And II is M/L(V) = 20.9(-10.1)(+13.9) M(circle dot)/L(V,circle dot). This value is similar to those of several Galactic dwarf spheroidal galaxies and is consistent with the presence of a massive dark halo in And II.