Magellan/M2FS Spectroscopy of the Reticulum 2 Dwarf Spheroidal Galaxy
arXiv:1504.03060 · doi:10.1088/0004-637X/808/2/108
Abstract
We present results from spectroscopic observations with the Michigan/Magellan Fiber System (M2FS) of 182 stellar targets along the line of sight to the newly-discovered `ultrafaint' object Reticulum 2 (Ret 2). For 38 of these targets, the spectra are sufficient to provide simultaneous estimates of line-of-sight velocity (, median random error km s), effective temperature (, K), surface gravity (, dex) and iron abundance ([Fe/H], dex). We use these results to confirm 18 stars as members of Ret 2. From the member sample we estimate a velocity dispersion of km s about a mean of km s in the solar rest frame ( km s in the Galactic rest frame), and a metallicity dispersion of dex about a mean of . These estimates marginalize over possible velocity and metallicity gradients, which are consistent with zero. Our results place Ret 2 on chemodynamical scaling relations followed by the Milky Way's dwarf-galactic satellites. Under assumptions of dynamic equilibrium and negligible contamination from binary stars---both of which must be checked with deeper imaging and repeat spectroscopic observations---the estimated velocity dispersion suggests a dynamical mass of enclosed within projected halflight radius pc, with mass-to-light ratio in solar units.
submitted to The Astrophysical Journal
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