The subgiant branch ofω Centauri seen through high-resolution spectroscopy

Author:

Pancino E.,Mucciarelli A.,Bonifacio P.,Monaco L.,Sbordone L.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 16 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. R-process-rich Stellar Streams in the Milky Way*;The Astrophysical Journal;2021-05-01

2. Omega Centauri: weak MgH band in red giants directly traces the helium content;Monthly Notices of the Royal Astronomical Society;2020-05-14

3. The Most Metal-poor Stars in Omega Centauri (NGC 5139);The Astronomical Journal;2020-05-07

4. Chemical Compositions of Field and Globular Cluster RR Lyrae Stars. II. ω Centauri∗;The Astrophysical Journal;2019-08-20

5. Accuracy and Precision of Industrial Stellar Abundances;Annual Review of Astronomy and Astrophysics;2019-08-18

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