2015MNRAS.448L..77D

We present a census of blue horizontal branch (BHB) and blue straggler (BS) stars belonging to dwarf galaxies and globular clusters, and compare these counts to that of the Milky Way stellar halo. We find, in agreement with earlier studies, that the ratio of BS-to-BHB stars in these satellite populations is dependent on stellar mass. Dwarf galaxies show an increasing BS-to-BHB ratio with luminosity. In contrast, globular clusters display the reverse trend, with NBS/NBHB ( ≲ 1) decreasing with luminosity. The faintest (L < 10⁵L_☉) dwarfs have similar numbers of BS and BHB stars (NBS/NBHB ∼ 1), whereas more-massive dwarfs tend to be dominated by BS stars (NBS/NBHB ∼ 2-40). We find that the BS-to-BHB ratio in the stellar halo is relatively high (NBS/NBHB ∼ 5-6), and thus inconsistent with the low ratios found in both ultra-faint dwarfs and globular clusters. Our results favour more-massive dwarfs as the dominant `building blocks' of the stellar halo, in good agreement with current predictions from Λ cold dark matter models.