A case against an X-shaped structure in the Milky Way young bulge
Martin Lopez-Corredoira

TL;DR
This study investigates the presence of an X-shaped structure in the Milky Way's bulge using young stellar populations, finding no evidence of such a structure contrary to previous claims based on red clump stars.
Contribution
It provides a novel analysis using young main-sequence stars to test the X-shape hypothesis, offering an alternative perspective to prior red clump star studies.
Findings
No double peak in stellar density along lines of sight.
Results challenge the existence of an X-shaped bulge in young stars.
Photometric uncertainties are insufficient to explain the lack of X-shape evidence.
Abstract
CONTEXT. A number of recent papers have claimed the discovery of an X-shape structure in the bulge of our Galaxy in the population of the red clumps. AIMS. We endeavor to analyze the stellar density of bulge stars in the same regions using a different stellar population that is characteristic of the young bulge ( Gyr). Particularly, we use F0-F5 main-sequence stars with distances derived through photometric parallax. METHODS. We extract these stars from extinction-corrected color-magnitude diagrams in the near-infrared of VISTA-VVV data in some bulge regions and calculate the densities along the line of sight. We take the uncertaintity in the photometric parallax and the contamination of other sources into account, and we see that these errors do not avoid the detection of a possible double peak along some lines of sight as expected for a X-shape bulge if it existed.…
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