The Metal-Poor Metallicity Distribution of the Ancient Milky Way
arXiv:2103.16642 · doi:10.3847/2041-8213/abd629
Abstract
We present a low metallicity map of the Milky Way consisting of 111,000 giants with [Fe/H] 0.75, based on public photometry from the second data release of the SkyMapper survey. These stars extend out to 7kpc from the solar neighborhood and cover the main Galactic stellar populations, including the thick disk and the inner halo. Notably, this map can reliably differentiate metallicities down to [Fe/H] , and thus provides an unprecedented view into the ancient, metal-poor Milky Way. Among the more metal-rich stars in our sample ([Fe/H] ), we recover a clear spatial dependence of decreasing mean metallicity as a function of scale height that maps onto the thick disk component of the Milky Way. When only considering the very metal-poor stars in our sample ([Fe/H] 2), we recover no such spatial dependence in their mean metallicity out to a scale height of kpc. We find that the metallicity distribution function (MDF) of the most metal-poor stars in our sample ( [Fe/H] ) is well fit with an exponential profile with a slope of [Fe/H] = 1.520.05, and shifts to [Fe/H] = 1.530.10 after accounting for target selection effects. For [Fe/H] , the MDF is largely insensitive to scale height out to kpc, showing that very and extremely metal-poor stars are in every galactic component.
arXiv comment9 pages, 5 figures; accepted for publication in ApJL. Minor corrections after acceptance addressing referee report for Chiti et al. ApJS submitted
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