Multiple Stellar Populations in Globular Clusters
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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...read more
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The GALAH Survey: Second Data Release
Sven Buder,Sven Buder,Martin Asplund,Ly Duong,Janez Kos,Karin Lind,Karin Lind,Melissa Ness,Melissa Ness,Sanjib Sharma,Joss Bland-Hawthorn,Joss Bland-Hawthorn,Andrew R. Casey,Gayandhi M. De Silva,Gayandhi M. De Silva,Valentina D'Orazi,Kenneth C. Freeman,Geraint F. Lewis,Jane Lin,Sarah L. Martell,Katharine J. Schlesinger,Jeffrey D. Simpson,Daniel B. Zucker,Daniel B. Zucker,Tomaž Zwitter,Anish M. Amarsi,Borja Anguiano,Daniela Carollo,Luca Casagrande,Klemen Čotar,P. L. Cottrell,P. L. Cottrell,Gary S. Da Costa,Xudong D. Gao,Michael R. Hayden,Jonathan Horner,Michael J. Ireland,Prajwal R. Kafle,Ulisse Munari,David M. Nataf,Thomas Nordlander,Dennis Stello,Dennis Stello,Yuan-Sen Ting,Yuan-Sen Ting,Yuan-Sen Ting,Gregor Traven,Fred Watson,Fred Watson,Robert A. Wittenmyer,Rosemary F. G. Wyse,David Yong,Joel C. Zinn,Maruša Žerjal +53 more
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Journal ArticleDOI
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
Sven Buder,Sven Buder,Sanjib Sharma,Janez Kos,Anish M. Amarsi,Thomas Nordlander,Karin Lind,Karin Lind,Sarah L. Martell,Martin Asplund,Joss Bland-Hawthorn,Andrew R. Casey,Gayandhi M. De Silva,Valentina D'Orazi,Kenneth C. Freeman,Michael R. Hayden,Geraint F. Lewis,Jane Lin,Katharine J. Schlesinger,Jeffrey D. Simpson,Dennis Stello,Dennis Stello,Dennis Stello,Daniel B. Zucker,Tomaž Zwitter,Kevin L. Beeson,Tobias Buck,Luca Casagrande,Jake T. Clark,Klemen Čotar,Gary S. Da Costa,Richard de Grijs,Richard de Grijs,Diane Feuillet,Diane Feuillet,Jonathan Horner,Prajwal R. Kafle,Shourya Khanna,Chiaki Kobayashi,F. Liu,Benjamin T. Montet,G. Nandakumar,David M. Nataf,Melissa Ness,Melissa Ness,Lorenzo Spina,Thor Tepper-García,Yuan-Sen Ting,Gregor Traven,Rok Vogrinčič,Robert A. Wittenmyer,Rosemary F. G. Wyse,Maruša Žerjal +52 more
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
Journal ArticleDOI
Evidence from the H3 Survey That the Stellar Halo Is Entirely Comprised of Substructure
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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.
Journal ArticleDOI
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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