Origin of chemically distinct discs in the Auriga cosmological simulations-Reference-Cited by-同舟云学术

Origin of chemically distinct discs in the Auriga cosmological simulations

Published:2017-11-23 Issue:3 Volume:474 Page:3629-3639
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Grand Robert J J^ORCID,Bustamante Sebastián^ORCID,Gómez Facundo A,Kawata Daisuke,Marinacci Federico^ORCID,Pakmor Rüdiger,Rix Hans-Walter,Simpson Christine M^ORCID,Sparre Martin,Springel Volker

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/474/3/3629/23002554/stx3025.pdf

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5. A FIRST CONSTRAINT ON THE THICK DISK SCALE LENGTH: DIFFERENTIAL RADIAL ABUNDANCES IN K GIANTS AT GALACTOCENTRIC RADII 4, 8, AND 12 kpc

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