Dynamics of Multiple Stellar Populations in Globular Clusters

球状星团中多个恒星族群的动力学

• 批准号: 2009193
• 负责人: Enrico Vesperini
• 金额: $ 36.1万
• 依托单位: Indiana University
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2020
• 资助国家: 美国
• 起止时间: 2020-09-01 至 2024-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2009193&HistoricalAwards=false
• 关键词: Dynamics; Multiple; Stellar; Populations; Globular

Globular clusters contain hundreds of thousands of stars confined in a region with a radius of only a few tens of light-years, much more densely packed than the region around our Sun. These clusters are among the oldest objects in the Universe, so they provide important clues to the formation of our Milky Way Galaxy. New observations have shown that stars within these clusters are not all formed at once, as previously thought, and they exhibit a range of chemical compositions. This group will conduct a theoretical study based on computer simulations of the formation and evolution of globular clusters. Students involved in this program will learn valuable computational and data visualization techniques that are broadly applicable beyond astronomy.Many observational studies have now provided strong evidence that most globular clusters host multiple stellar populations characterized by different chemical properties. This discovery represents a major shift in the common view of globular clusters as systems composed of stars with the same chemical composition. The investigators will model the cluster’s dynamical history, so they can trace motions of the stars back to the formation of the stars. They will model of the formation and dynamical changes with time of multiple populations of stars in these globular clusters. This program will carry out extensive simulations to address: 1) the formation of multiple-population clusters and the characterization of the initial structural and kinematical properties of first- and second-generation stars, 2) the early and long-term evolution of the dynamical properties of first- and second-generation stars, 3) the role of internal dynamical processes and the external tidal field of the host galaxy in the evolution of multiple-population clusters, 4) the evolution of the fundamental properties of the cluster's stellar content and how they are affected by the different initial structural properties of multiple populations.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

球状星团包含数十万颗恒星，它们被限制在一个半径只有几十光年的区域内，比我们太阳周围的区域要密集得多。这些星团是宇宙中最古老的天体之一，因此它们为我们银河系的形成提供了重要线索。新的观测表明，这些星团中的恒星并不像以前认为的那样是一次形成的，它们表现出一系列的化学成分。 该小组将根据球状星团形成和演化的计算机模拟进行理论研究。 参与该计划的学生将学习有价值的计算和数据可视化技术，这些技术广泛适用于天文学之外。许多观测研究现在提供了强有力的证据，表明大多数球状星团拥有多个具有不同化学性质的恒星群。这一发现代表了球状星团是由具有相同化学成分的恒星组成的系统的共同观点的重大转变。 研究人员将模拟星团的动力学历史，这样他们就可以追踪恒星的运动，追溯到恒星的形成。 他们将模拟这些球状星团中多个恒星群体的形成和动态变化。该计划将进行广泛的模拟，以解决：1）多星族星团的形成以及第一代和第二代恒星初始结构和运动学性质的表征，2）第一代和第二代恒星动力学性质的早期和长期演化，3）宿主星系的内部动力学过程和外部潮汐场在多居群星系团演化中的作用，四、该奖项反映了美国国家科学基金会的法定使命，通过使用基金会的知识价值和更广泛的影响审查标准进行评估，认为值得支持。

项目成果

Constraining the original composition of the gas forming first-generation stars in globular clusters

限制球状星团中形成第一代恒星的气体的原始成分

• DOI: 10.1093/mnras/stac734
• 发表时间: 2022
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Legnardi, M V;Milone, A P;Armillotta, L;Marino, A F;Cordoni, G;Renzini, A;Vesperini, E;D’Antona, F;McKenzie, M;Yong, D
• 通讯作者: Yong, D

The role of rotation on the formation of second generation stars in globular clusters

自转对球状星团第二代恒星形成的作用

• DOI: 10.1093/mnras/stac2328
• 发表时间: 2022
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Lacchin, E.;Calura, F.;Vesperini, E.;Mastrobuono-Battisti, A.
• 通讯作者: Mastrobuono-Battisti, A.

Light Element Abundances and Multiple Populations in M53

• DOI: 10.3847/1538-3881/abf04d
• 发表时间: 2018-05
• 期刊: The Astronomical Journal
• 作者: J. Gerber;E. Friel;E. Vesperini

Sub-parsec resolution cosmological simulations of star-forming clumps at high redshift with feedback of individual stars

利用单个恒星的反馈对高红移恒星形成团块进行亚秒差距分辨率宇宙学模拟

• DOI: 10.1093/mnras/stac2387
• 发表时间: 2022
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Calura, F.;Lupi, A.;Rosdahl, J.;Vanzella, E.;Meneghetti, M.;Rosati, P.;Vesperini, E.;Lacchin, E.;Pascale, R.;Gilli, R.
• 通讯作者: Gilli, R.

3D core kinematics of NGC 6362: central rotation in a dynamically evolved globular cluster

NGC 6362 的 3D 核心运动学：动态演化的球状星团中的中心旋转

• DOI: 10.1093/mnras/stab1257
• 发表时间: 2021
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Dalessandro, Emanuele;Raso, Silvia;Kamann, Sebastian;Bellazzini, Michele;Vesperini, Enrico;Bellini, Andrea;Beccari, Giacomo
• 通讯作者: Beccari, Giacomo