The Galactic thin and thick disks in the context of galaxy formation

Author:

Bensby Thomas,Feltzing Sofia

Abstract

AbstractWe have obtained high-resolution spectra and carried out a detailed elemental abundance analysis for a new sample of 899 F and G dwarf stars in the Solar neighbourhood. The results allow us to, in a multi-dimensional space consisting of stellar ages, detailed elemental abundances, and full kinematic information for the stars, study and trace their respective origins. Here we briefly address selection criteria and discuss how to define a thick disc star. The results are discussed in the context of galaxy formation.

Publisher

Cambridge University Press (CUP)

Subject

Astronomy and Astrophysics,Space and Planetary Science

Cited by 8 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. GALAH ve Gaia Verileriyle Samanyolu'nda Metal Bolluğu Gradyent Araştırması;Turkish Journal of Astronomy and Astrophysics;2022-02-08

2. Heating of Milky Way disc stars by dark matter fluctuations in cold dark matter and fuzzy dark matter paradigms;Monthly Notices of the Royal Astronomical Society;2019-02-22

3. TheGaia-ESO Survey: the Galactic thick to thin disc transition;Astronomy & Astrophysics;2014-07

4. Exploring the Milky Way stellar disk;Astronomy & Astrophysics;2014-02

5. How can star formation be sustained?;Proceedings of the International Astronomical Union;2013-05

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