The cluster Terzan 5 as a remnant of a primordial building block of the Galactic bulge
F. R. Ferraro (1), E. Dalessandro (1), A. Mucciarelli (1), G. Beccari, (2), R. M. Rich (3), L. Origlia (4), B. Lanzoni (1), R. T. Rood (5), E., Valenti (6,7), M. Bellazzini (4), S. M. Ransom (8), G. Cocozza (4) ((1), Department of Astronomy, University of Bologna, (2) ESA

TL;DR
This paper reveals that Terzan 5, a globular cluster in the Galactic bulge, contains multiple stellar populations with different ages and iron content, suggesting it is a remnant of a primordial galaxy building block.
Contribution
It provides evidence that Terzan 5 is a surviving remnant of a primordial bulge building block, with multiple stellar populations, unlike typical globular clusters.
Findings
Terzan 5 has two stellar populations with different iron content.
Terzan 5 shows different ages among its stellar populations.
Supports the idea of Terzan 5 as a primordial bulge remnant.
Abstract
Globular star clusters are compact and massive stellar systems old enough to have witnessed the entire history of our Galaxy, the Milky Way. Although recent results suggest that their formation may have been more complex than previously thought, they still are the best approximation to a stellar population formed over a relatively short time scale (less than 1 Gyr) and with virtually no dispersion in the iron content. Indeed, only one cluster-like system (omega Centauri) in the Galactic halo is known to have multiple stellar populations with a significant spread in iron abundance and age4,5. Similar findings in the Galactic bulge have been hampered by the obscuration arising from thick and varying layers of interstellar dust. Here we report that Terzan 5, a globular-cluster-like system in the Galactic bulge, has two stellar populations with different iron content and ages. Terzan 5…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
