# Globular cluster candidates in the Galactic bulge: Gaia and VVV view of the latest discoveries

## TL;DR

This paper introduces a new method combining Gaia and VVV data to reliably confirm star cluster candidates by analyzing their spatial distribution, motion, and color-magnitude features, successfully identifying a new cluster and validating some candidates.

## Contribution

The paper presents a novel multi-dimensional approach for confirming star clusters, improving the reliability of candidate identification using combined spatial, kinematic, and photometric data.

## Key findings

- Successfully recovered known star clusters in the bulge region.
- Detected one new likely old star cluster.
- Confirmed only two out of 93 candidate clusters as real groups.

## Abstract

Thanks to the recent wide-area photometric surveys, the number of star cluster candidates have risen exponentially in the last few years. Most detections, however, are based only on the presence of an overdensity of stars in a given region, or an overdensity of variable stars, regardless of their distance. As candidates, their detection has not been dynamically confirmed. Therefore, it is currently unknown how many, and which ones, of the published candidates, are true clusters, and which ones are chance alignments. We present a method to detect and confirm star clusters based on the spatial distribution, coherence in motion and appearance on the color-magnitude diagram. We explain and apply it to one new star cluster, and several candidate star clusters published in the literature. The presented method is based on data from the Second Data Release of Gaia complemented with data from the VISTA Variables in the V\'ia L\'actea survey for the innermost bulge regions. It consists of a nearest neighbors algorithm applied simultaneously over spatial coordinates, star color, and proper motions, in order to detect groups of stars that are close in the sky, move coherently and define narrow sequences in the color-magnitude diagram, such as a young main sequence or a red giant branch. When tested in the bulge area ($-10<\ell\ {\rm (deg)}<+10$; $-10<b\ {\rm (deg)}<+10$) the method successfully recovered several known young and old star clusters. We report here the detection of one new, likely old star cluster, while deferring the others to a forthcoming paper. Additionally, the code has been applied to the position of 93 candidate star clusters published in the literature. As a result, only two of them are confirmed as coherently moving groups of stars at their nominal positions.