Reinforcing the link between the double red clump and the X-shaped bulge of the Milky Way
O. A. Gonzalez, M. Zoccali, Victor P. Debattista, J. Alonso-Garc\'ia,, E. Valenti, D. Minniti

TL;DR
This paper confirms that the double red clump in the Milky Way bulge is due to an X-shaped structure, dismissing alternative explanations involving multiple stellar populations, based on observational evidence.
Contribution
It provides observational evidence supporting the X-shaped bulge interpretation over alternative stellar population scenarios.
Findings
Double red clump aligns with X-shaped bulge distance distribution.
Alternative multiple population explanation is inconsistent with observations.
Key properties of the red clump are crucial for understanding bulge structure.
Abstract
The finding of a double red clump in the luminosity function of the Milky Way bulge has been interpreted as evidence for an X-shaped structure. Recently, an alternative explanation has been suggested, where the double red clump is an effect of multiple stellar populations in a classical spheroid. In this letter we provide an observational assessment of this scenario and show that it is not consistent with the behaviour of the red clump across different lines of sight, particularly at high distances from the Galactic plane. Instead, we confirm that the shape of the red clump magnitude distribution closely follows the distance distribution expected for an X-shaped bulge at critical Galactic latitudes. We also emphasize some key observational properties of the bulge red clump that should not be neglected in the search for alternative scenarios.
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