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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…

Terzan 5 is a stellar system located in the Galactic Bulge, at a distance of 5.9 kpc. Recent discoveries show that it hosts two stellar populations with different iron abundance ({\Delta}[Fe/H]=0.5). Such a large difference has been…

Astrophysics of Galaxies · Physics 2013-01-14 D. Massari , F. R. Ferraro , E. Dalessandro , B. Lanzoni , A. Mucciarelli , L. Origlia

Terzan 5 is a stellar system in the Galactic bulge commonly catalogued as a globular cluster. Through dedicated NIR photometry and spectroscopy we have discovered that it harbors two main stellar populations defining two distinct red clumps…

Astrophysics of Galaxies · Physics 2013-11-21 Barbara Lanzoni , the Cosmic-Lab Team

Terzan 5 is a stellar system located in the inner Bulge of the Galaxy and has been historically catalogued as a globular cluster. However, recent photometric (Ferraro et al. 2009) and spectroscopic (Origlia et al. 2011; Origlia et al. 2013)…

Astrophysics of Galaxies · Physics 2014-01-17 Davide Massari , F. R. Ferraro , A. Mucciarelli , L. Origlia , E. Dalessandro , B. Lanzoni

The formation and evolution of galaxy bulges is one of the most debated topics in the modern astrophysics. One approach to address this issue is to look at the Galactic bulge since it is the closest. According to some theoretical models,…

Astrophysics of Galaxies · Physics 2014-12-19 Davide Massari

Terzan 5 is a heavily obscured stellar system located in the inner Galaxy. It has been postulated to be a stellar relic, a Bulge Fossil Fragment witnessing the complex history of the assembly of the Milky Way bulge. In this paper, we follow…

The Galactic bulge is dominated by an old, metal rich stellar population. The possible presence and the amount of a young (a few Gyr old) minor component is one of the major issues debated in the literature. Recently, the bulge stellar…

Astrophysics of Galaxies · Physics 2016-09-21 F. R. Ferraro , D. Massari , E. Dalessandro , B. Lanzoni , L. Origlia , R. M. Rich , A. Mucciarelli , -

The James Webb Space Telescope provides an exciting opportunity to investigate stellar systems located in heavily obscured regions like the Galactic bulge. Possibly, the most enigmatic among them is Terzan 5: long classified as a globular…

Over the past decade the discovery of three unique stellar populations and a large number of confirmed pulsars within the globular cluster Terzan 5 has raised questions over its classification. Using the long-term radio pulsar timing of 36…

Solar and Stellar Astrophysics · Physics 2017-08-30 Brian Prager , Scott Ransom , Paulo Freire , Jason Hessels , Ingrid Stairs , Phil Arras , Mario Cadelano

We report on the discovery of 3 metal-poor giant stars in Terzan 5, a complex stellar system in the the Galactic bulge, known to have two populations at [Fe/H]=-0.25 and +0.3. For these 3 stars we present new echelle spectra obtained with…

Astrophysics of Galaxies · Physics 2015-06-17 L. Origlia , D. Massari , R. M. Rich , A. Mucciarelli , F. R. Ferraro , E. Dalessandro , B. Lanzoni

It has been proposed that the globular cluster-like system Terzan 5 is the surviving remnant of a primordial building block of the Milky Way bulge, mainly due to the age/metallicity spread and the distribution of its stars in the…

We address the chemical link between Terzan 5 (hereafter Ter5) and the Bulge, as probed by the observed distributions of [$\alpha$/Fe] abundance ratios with varying [Fe/H] and by suitable statistical tests to evaluate their significance. We…

Astrophysics of Galaxies · Physics 2025-04-30 L. Origlia , F. R. Ferraro , C. Fanelli , B. Lanzoni , D. Massari , E. Dalessandro , C. Pallanca

We present the chemical abundance analysis of 33 red giant stars belonging to the complex stellar system Terzan 5. We confirm the discovery of two stellar populations (Ferraro et al. 2009, Nature, 462,483) with distinct iron abundances: a…

Astrophysics of Galaxies · Physics 2015-05-20 L. Origlia , R. M. Rich , F. R. Ferraro , B. Lanzoni , M. Bellazzini , E. Dalessandro , A. Mucciarelli , E. Valenti , G. Beccari

The formation and evolutionary processes of galaxy bulges are still unclear, and the presence of young stars in the bulge of the Milky Way is largely debated. We recently demonstrated that Terzan 5, in the Galactic bulge, is a complex…

Recent observational studies have demonstrated that the complex stellar system Terzan 5 (Ter 5) harbours multiple populations of stars. Several models have attempted to interpret the large age difference of several Gyrs between the dominant…

Astrophysics of Galaxies · Physics 2018-06-14 Madeleine McKenzie , Kenji Bekki

Terzan5 is the globular cluster (GC)-like stellar system harboring the largest known population of MSPs. Using the Multi-Conjugate Adaptive Optics demonstrator MAD at the ESO - VLT, we recently obtained a superb (K, J - K) color-magnitude…

Astrophysics of Galaxies · Physics 2015-05-20 Francesco R. Ferraro

Context. Terzan 5 and Liller 1 are the only bulge stellar clusters hosting multi-iron and multi-age stellar populations. They are therefore claimed to constitute a novel class of astrophysical objects: the fossils of massive star-forming…

We present new determinations of the iron abundance for 220 stars belonging to the stellar system Terzan 5 in the Galactic bulge. The spectra have been acquired with FLAMES at the Very Large Telescope of the European Southern Observatory…

Terzan 5 is a rich globular cluster within the galactic bulge that contains 39 known millisecond pulsars, the largest known population of any globular cluster. The Terzan 5 pulsars are faint, so that individual observations of most of the…

By exploiting two sets of high-resolution images obtained with HST ACS/WFC over a baseline of ~10 years we have measured relative proper motions of ~70,000 stars in the stellar system Terzan 5. The results confirm the membership of the…

Astrophysics of Galaxies · Physics 2017-12-06 Davide Massari , E. Dalessandro , F. R. Ferraro , P. Miocchi , A. Bellini , L. Origlia , B. Lanzoni , R. M. Rich , A. Mucciarelli
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