The formation of the milky way halo and its dwarf satellites: a NLTE-1D abundance analysis. IV. Segue 1, Triangulum ii , and Coma Berenices UFDs

The formation of the milky way halo and its dwarf satellites: a NLTE-1D abundance analysis. IV. Segue 1, Triangulum ii , and Coma Berenices UFDs

ABSTRACT We present atmospheric parameters and abundances for chemical elements from carbon to barium in metal-poor stars in Segue 1 (seven stars), Coma Berenices (three stars), and Triangulum ii (one star) ultrafaint dwarf galaxies (UFDs). The effective temperatures rely on new photometric observa...

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Bibliographic Details
Main Authors: Sitnova, TM, Mashonkina, LI, Tatarnikov, AM, Voziakova, OV, Burlak, MA, Pakhomov, Yu V, Jablonka, P, Neretina, MD, Frebel, A
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:English
Published: Oxford University Press (OUP) 2022
Online Access:https://hdl.handle.net/1721.1/141837

Internet

https://hdl.handle.net/1721.1/141837

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