Abstract
We use a sample of 938 red clump giant stars located in the direction of the Galactic long bar to study the chemistry of Milky Way bar stars. Kinematically separating stars on bar orbits from stars with inner disc orbits, we find that stars on bar-like orbits are more metal rich with a mean iron abundance of ⟨[Fe/H]⟩ = +0.30 compared to ⟨[Fe/H]⟩ = +0.03 for the inner disc. Spatially selecting bar stars is complicated by a strong vertical metallicity gradient of −1.1 dex kpc−1, but we find the metallicity distribution varies in a manner consistent with our orbital selection. Our results have two possible interpretations. The first is that the most metal rich stars in the inner Galaxy pre-existed the bar, but were kinematically cold at the time of bar formation and therefore more easily captured onto bar orbits when the bar formed. The second is that the most metal rich stars formed after the bar, either directly onto the bar following orbits or were captured by the bar after their formation.
Highlights
The vertically extended bulge region of the Milky Way is shaped as a box/peanut bulge (B/P bulge; Lopez-Corredoira et al 2005; Saito et al 2011; Wegg & Gerhard 2013)
We find that the metallicity distribution function (MDF) of the stars in the bar and in front of the bar are very similar, while those behind the bar are more metal poor
We find that the bar of the Milky Way outside the B/P bulge is more metal rich than the inner disc
Summary
The vertically extended bulge region of the Milky Way is shaped as a box/peanut bulge (B/P bulge; Lopez-Corredoira et al 2005; Saito et al 2011; Wegg & Gerhard 2013) Such shapes naturally arise in simulations of barred galaxies We study the chemistry of stars in the long bar of the Milky Way from a spectroscopic sample of ∼2500 stars. From these we select ∼1000 red clump giants (RCGs) whose standard candle nature provides ∼10% accurate distances. 4 we make spatial and kinematic selections of stars that are likely to be bar stars and show the chemistry of these bar stars compared to the inner disc of the Milky Way. In Sect.
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