The small boxy/peanut structure of the Milky Way traced by old stars

Abstract

We analyse the positions of RR Lyrae stars in the central region of the Milky Way. In addition to the overall bar shape detected previously, we find evidence for a peanut shaped structure, in form of overdensities near $\ell =-2$ deg and $1$ deg at $b\sim -3.5$ deg. The corresponding physical distance between the two peaks of the peanut is $\sim 0.7$ kpc, significantly shorter than that found from near-IR images (3.3 kpc) and red-clump stars. Qualitatively this is expected from `fractionation' of bar orbits, which we demonstrate to be matched in a simulation of an inside-out growing disc subsequently forming a bar.

6 pages, 5 figures, accepted to MNRAS

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Cited by in corpus (3)

• The OGLE Collection of Variable Stars. Nearly 66,000 Mira stars in the Milky Way
• A three-dimensional map of the Milky Way using 66,000 Mira variable stars
• Age-morphology dependence of the Milky Way boxy/peanut bulge seen in Mira variables