@article{a3f9e888080941feadcabcdbfced11a2,
title = "The Pristine survey -- XVII. The C-19 stream is dynamically hot and more extended than previously thought",
abstract = " The C-19 stream is the most metal poor stellar system ever discovered, with a mean metallicity \$[Fe/H] = -3.38\textbackslash{}pm0.06\$. Its low metallicity dispersion (\$\textbackslash{}sigma\_\{\textbackslash{}rm [Fe/H]\}\$ \$",
keywords = "astro-ph.GA",
author = "Zhen Yuan and Martin, \{Nicolas F.\} and Ibata, \{Rodrigo A.\} and Elisabetta Caffau and Piercarlo Bonifacio and Mashonkina, \{Lyudmila I.\} and Rapha{\"e}l Errani and Amandine Doliva-Dolinsky and Else Starkenburg and Venn, \{Kim A.\} and Anke Arentsen and Aguado, \{David S.\} and Michele Bellazzini and Benoit Famaey and Morgan Fouesneau and Hern{\'a}ndez, \{Jonay I. Gonz{\'a}lez\} and Pascale Jablonka and Carmela Lardo and Khyati Malhan and Navarro, \{Julio F.\} and Janssen, \{Rub{\'e}n S{\'a}nchez\} and Federico Sestito and Thomas, \{Guillaume F.\} and Akshara Viswanathan and Sara Vitali",
note = "7 pages, 6 figures, accepted to MNRAS. The C-19 member list is published via https://github.com/zyuan-astro/C-19",
year = "2022",
month = mar,
day = "4",
doi = "10.1093/mnras/stac1399",
language = "Undefined/Unknown",
journal = "Monthly Notices of the Royal Astronomical Society (MNRAS)",
issn = "0035-8711",
publisher = "Oxford University Press (OUP)",
}