English

A stellar stream remnant of a globular cluster below the metallicity floor

Astrophysics of Galaxies 2022-01-06 v1

Abstract

Stellar ejecta gradually enrich the gas out of which subsequent stars form, making the least chemically enriched stellar systems direct fossils of structures formed in the early universe. Although a few hundred stars with metal content below one thousandth of the solar iron content are known in the Galaxy, none of them inhabit globular clusters, some of the oldest known stellar structures. These show metal content of at least ~0.2 percent of the solar metallicity ([Fe/H] > -2.7). This metallicity floor appears universal and it has been proposed that proto-galaxies that merge into the galaxies we observe today were simply not massive enough to form clusters that survived to the present day. Here, we report the discovery of a stellar stream, C-19, whose metallicity is less than 0.05 per cent the solar metallicity ([Fe/H]=-3.38 +/- 0.06 (stat.) +/- 0.20 (syst.)). The low metallicity dispersion and the chemical abundances of the C-19 stars show that this stream is the tidal remnant of the most metal-poor globular cluster ever discovered, and significantly below the purported metallicity floor: clusters with significantly lower metallicities than observed today existed in the past and contributed their stars to the Milky Way halo.

Keywords

Cite

@article{arxiv.2201.01309,
  title  = {A stellar stream remnant of a globular cluster below the metallicity floor},
  author = {Nicolas F. Martin and Kim A. Venn and David S. Aguado and Else Starkenburg and Jonay I. González Hernández and Rodrigo A. Ibata and Piercarlo Bonifacio and Elisabetta Caffau and Federico Sestito and Anke Arentsen and Carlos Allende Prieto and Raymond G. Carlberg and Sébastien Fabbro and Morgan Fouesneau and Vanessa Hill and Pascale Jablonka and Georges Kordopatis and Carmela Lardo and Khyati Malhan and Lyudmila I. Mashonkina and Alan W. McConnachie and Julio F. Navarro and Rubén Sánchez Janssen and Guillaume F. Thomas and Zhen Yuan and Alessio Mucciarelli},
  journal= {arXiv preprint arXiv:2201.01309},
  year   = {2022}
}

Comments

14 pages, 6 figures, 5 tables. Nature, accepted