APOGEE discovery of a chemically atypical star disrupted from NGC\,6723 and captured by the Milky Way bulge

FERNANDEZ-TRINCADO,+15, A.E. PIATTI, +12

ASTRONOMY AND ASTROPHYSICS

EDP SCIENCES S A

Lugar: Paris; Año: 2021 vol. 647 p. 1 - 17

0004-6361

The central (?bulge?) region of the Milky Way is teeming with a significant fraction of mildly metal-deficient stars with atmospheres that are strongly enriched in cyanogen (12C14N). Also known as nitrogen-enhanced stars, some of these objects are hypothesized to be relics of the ancient assembly history of the Milky Way. Although the chemical similarity of nitrogen-enhanced stars to the unique chemical patterns observed in globular clusters has been observed, a direct connection between field stars and globular clusters has not yet been proven. In this work, we report on high-resolution, near-infrared spectroscopic observations of the bulge globular cluster NGC 6723, and the serendipitous discovery of a star, 2M18594405−3651518, located outside the cluster (near the tidal radius) but moving on a similar orbit, providing the first clear evidence of a star that was very likely once a cluster member and has recently been ejected. Its nitrogen abundance ratio ([N/Fe]􏰀 +0.94) is well above the typical Galactic field-star levels, and it exhibits noticeable enrichment in the heavy s-process elements (Ce, Nd, and Yb), along with moderate carbon enrichment, all characteristics of known examples in globular clusters. This result suggests that some of the nitrogen-enhanced stars in the bulge likely originated from tidal disruption of globular clusters.