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Multiple Stellar Populations in Globular Clusters

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TLDR
In this paper, star-to-star variations in specific elements (e.g., He, C, N, O, Na, Al) that bear the hallmark of high-temperature H-burning are discussed.
Abstract
Globular clusters (GCs) exhibit star-to-star variations in specific elements (e.g., He, C, N, O, Na, Al) that bear the hallmark of high-temperature H-burning. These abundance variations can be obse...

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The GALAH Survey: Second Data Release

TL;DR: In this paper, the authors present the GALAH second public data release (GALAH DR2) containing 342 682 stars and use the physics-driven spectrum synthesis of Spectroscopy Made Easy (SME) to derive stellar labels.
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The formation and assembly history of the Milky Way revealed by its globular cluster population

TL;DR: In this paper, the formation and assembly history of the Milky Way (MW) was reconstructed from the age-metallicity distribution of 96 Galactic globular clusters (GCs) to infer the merger tree of the MW.
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The GALAH+ survey: Third data release

TL;DR: In this paper, the accepted manuscript version of an article which has been published in final form at https://doi.org/10.1093/mnras/stab1242
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Evidence from the H3 Survey That the Stellar Halo Is Entirely Comprised of Substructure

TL;DR: In this paper, the authors presented a comprehensive inventory of structure within 50 kpc from the Galactic center using a sample of 5684 giants at $|b|>40^{\circ}$ and $|Z|>2$ kpc.
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Angular Momentum Transport in Stellar Interiors

TL;DR: In this paper, it was shown that stars lose a significant amount of angular momentum between birth and death, implying that efficient processes transporting it from the core to the surface are active Space asteroseismology delive.
References
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The E-MOSAICS project: simulating the formation and co-evolution of galaxies and their star cluster populations

TL;DR: In this article, the authors introduce the MOdelling Star cluster population Assembly In Cosmological Simulations within EAGLE (E-MOSAICS) project, which incorporates models describing the formation, evolution, and disruption of star clusters into the eagle galaxy formation simulations, enabling the examination of the co-evolution of star cluster and their host galaxies in a fully cosmological context.
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