Descendants of the first stars: the distinct chemical signature of second-generation stars

ABSTRACT. Extremely metal-poor (EMP) stars in the Milky Way (MW) allow us to infer the properties of their progenitors by comparing their chemical composition

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Bibliographic Details
Main Authors:	Hartwig, Tilman (Author) , Yoshida, Naoki (Author) , Magg, Mattis (Author) , Frebel, Anna (Author) , Glover, Simon (Author) , Gómez, Facundo A. (Author) , Griffen, Brendan (Author) , Ishigaki, Miho N. (Author) , Ji, Alexander P. (Author) , Klessen, Ralf S. (Author) , O’Shea, Brian W. (Author) , Tominaga, Nozomu (Author)
Format:	Article (Journal)
Language:	English
Published:	07 May 2018
In:	Monthly notices of the Royal Astronomical Society Year: 2018, Volume: 478, Issue: 2, Pages: 1795-1810
ISSN:	1365-2966
DOI:	10.1093/mnras/sty1176
Online Access:	Verlag, Volltext: https://doi.org/10.1093/mnras/sty1176 Verlag: https://academic.oup.com/mnras/article/478/2/1795/4993535
Author Notes:	Tilman Hartwig, Naoki Yoshida, Mattis Magg, Anna Frebel, Simon C. O. Glover, Facundo A. Gómez, Brendan Griffen, Miho N. Ishigaki, Alexander P. Ji, Ralf S. Klessen, Brian W. O’Shea, and Nozomu Tominaga

Description
Summary:	ABSTRACT. Extremely metal-poor (EMP) stars in the Milky Way (MW) allow us to infer the properties of their progenitors by comparing their chemical composition
Item Description:	Gesehen am 16.10.2019
Physical Description:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/sty1176