Exploring Halo Substructure with Giant Stars: The Dynamics and Metallicity of the Dwarf Spheroidal in Bootes

摘要

We report the results of a spectroscopic study of the Bootes (Boo) dwarf spheroidal (dSph) galaxy carried out with the WIYN telescope and the Hydra multifiber spectrograph. Radial velocities have been measured for 58 Boo candidate stars selected to have magnitudes and colors consistent with its red and asymptotic giant branches. Within the 13 arcmin half-light radius, seven members of Boo yield a systemic velocity of V_sun=95.6+-3.4 km/s and a velocity dispersion of 6.6+-2.3 km/s. This implies a mass on the order of 1 x 10^7 M_sun, similar to the inferred masses of other Galactic dSphs. Adopting a total Boo luminosity of L=1.6 x 10^4 L_sun to L=8.6 x 10^4 L_sun implies M/L~680 to 130, making Boo, the most distorted known Milky Way dwarf galaxy, potentially also the darkest. In addition, from the spectra of Boo member stars we estimate its metallicity to be [Fe/H] ~-2.5, which makes it the most metal poor dSph known to date.