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The Assembly History of M87 through Radial Variations in Chemical Abundances of Its Field Star and Globular Cluster Populations

机译：M87的装配历史通过其现场明星和球状群体化学丰富的径向变化

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Alexa Villaume; Daniel Foreman-Mackey; Aaron J. Romanowsky; Jean Brodie; Jay Strader;
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1. The Assembly History of M87 through Radial Variations in Chemical Abundances of Its Field Star and Globular Cluster Populations [J] . Alexa Villaume, Daniel Foreman-Mackey, Aaron J. Romanowsky, The Astrophysical journal . 2020,第2期

机译：M87的组装历史通过其野外明星和球状群体化学丰富的径向变化
2. THE FORMATION OF GLOBULAR CLUSTER SYSTEMS IN MASSIVE ELLIPTICAL GALAXIES: GLOBULAR CLUSTER MULTIMODALITY FROM RADIAL VARIATION OF STELLAR POPULATIONS [J] . Antonio Pipino, Thomas H. Puzia, Francesca Matteucci The Astrophysical journal . 2007,第1Pt1期

机译：大规模椭圆星系中的球状团簇系统的形成：来自星状群体径向变化的球状团簇多态性
3. The Formation of Globular Cluster Systems in Massive Elliptical Galaxies: Globular Cluster Multimodality from Radial Variation of Stellar Populations [J] . Antonio Pipino, Thomas H. Puzia, Francesca Matteucci The Astrophysical journal . 2007,第1期

机译：大规模椭圆星系中球状星团系统的形成：恒星群体径向变化的球状星团多模态
4. Spectroscopic studies of stellar populations in globular clusters and field stars: Implications for globular cluster and Milky Way halo formation [C] . Raffaele Gratton Symposium of the International Astronomical Union;International Astronomical Union., Symposium . 2020

机译：球状簇和田径恒星群体的光谱研究：球状簇的影响和银河系晕染
5. Where have all the Ap stars gone? Rotation, chemical abundances and magnetic fields of Ap stars in nearby open clusters. [D] . Silvester, James. 2007

机译：所有Ap明星都去了哪里？附近疏散星团中Ap星的自转，化学丰度和磁场。
6. On a Possible Relation between Globular Clusters and Stars of High Velocity [O] . J. H. Oort 2015

机译：球状星团与高速恒星之间的可能关系
7. Evolution of long-lived globular cluster stars. II. Sodium abundance variations on the asymptotic giant branch as a function of globular cluster age and metallicity [O] . Charbonnel C, Chantereau W 100

机译：长寿命球状星团的演化。二。渐近巨枝上钠的丰度变化与球状团簇年龄和金属性的关系

The Assembly History of M87 through Radial Variations in Chemical Abundances of Its Field Star and Globular Cluster Populations

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