The cluster Terzan 5 as a remnant of a primordial building block of the Galactic bulge

F. R. Ferraro (), E. Dalessandro, A. Mucciarelli, G. Beccari, R. M. Rich, L. Origlia, B. Lanzoni, R. T. Rood, E. Valenti, M. Bellazzini, S. M. Ransom and G. Cocozza
Additional contact information
F. R. Ferraro: University of Bologna, Via Ranzani, 1, 40127 Bologna, Italy
E. Dalessandro: University of Bologna, Via Ranzani, 1, 40127 Bologna, Italy
A. Mucciarelli: University of Bologna, Via Ranzani, 1, 40127 Bologna, Italy
G. Beccari: ESA, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands
R. M. Rich: Math-Sciences 8979, UCLA, Los Angeles, California 90095-1562, USA
L. Origlia: INAF-Osservatorio Astronomico di Bologna, Via Ranzani
B. Lanzoni: University of Bologna, Via Ranzani, 1, 40127 Bologna, Italy
R. T. Rood: University of Virginia, PO Box 400325, Charlottesville, Virginia 22904, USA
E. Valenti: European Southern Observatory, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago, Chile
M. Bellazzini: INAF-Osservatorio Astronomico di Bologna, Via Ranzani
S. M. Ransom: National Radio Astronomy Observatory, Charlottesville, Virginia 22903, USA
G. Cocozza: INAF-Osservatorio Astronomico di Bologna, Via Ranzani

Nature, 2009, vol. 462, issue 7272, 483-486

Abstract: Globular clusters a mixed bag The globular star clusters that orbit the Milky Way are regarded as the best approximations we have of stellar populations of uniform age and identical composition, recording stellar evolution since the birth of our Galaxy. The most luminous of these clusters though, ω Centauri, has long been recognized as an exception to this trend, containing multiple stellar populations with a significant spread in iron abundance and ages. Two groups report the discovery of further global clusters with mixed populations. Lee et al. confirm the suspicion that the massive global cluster M22 contains distinct multiple populations with different calcium abundances, as do several other clusters in their sample. Ferraro et al. report that Terzan 5, a globular cluster-like system in the Galactic bulge, has two populations with different iron content and ages. These findings suggest that ω Cen, M22, Terzan 5 and other similar clusters are the relics of dwarf galaxies and other primordial bodies that merged to eventually form the Milky Way.

Date: 2009
References: Add references at CitEc
Citations:

Downloads: (external link)
https://www.nature.com/articles/nature08581 Abstract (text/html)
Access to the full text of the articles in this series is restricted.

Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.

Export reference: BibTeX RIS (EndNote, ProCite, RefMan) HTML/Text

Persistent link: https://EconPapers.repec.org/RePEc:nat:nature:v:462:y:2009:i:7272:d:10.1038_nature08581

Ordering information: This journal article can be ordered from
https://www.nature.com/

DOI: 10.1038/nature08581

Access Statistics for this article

Nature is currently edited by Magdalena Skipper

More articles in Nature from Nature
Bibliographic data for series maintained by Sonal Shukla () and Springer Nature Abstracting and Indexing ().