Postdoctoral Fellowship: AAPF: From Dense Clusters to OB Associations: Tracing the Impact of Dynamics on Multiplicity beyond 10 AU in the Orion Complex
Postdoctoral Fellowship: AAPF: From Dense Clusters to OB Associations: Tracing the Impact of Dynamics on Multiplicity beyond 10 AU in the Orion Complex
批准号:
2303911
负责人:
Matthew De Furio
金额:
$33.0万
依托单位:
依托单位国家:
美国
项目类别:
Fellowship Award
财政年份:
2023
资助国家:
美国
项目状态:
未结题
起止时间:
2023-09-01 至 2026-08-31
中文摘要
Matthew De Furio被授予美国国家科学基金会天文学和天体物理学奖学金,在德克萨斯大学奥斯汀分校开展研究和教育项目。De Furio将在四个不同的恒星形成区域(从低密度非束缚区到高密度束缚区)观察数百颗恒星,以识别双星和高阶多重系统。这项工作的结果将告诉我们对恒星形成过程的理解,并探索恒星诞生环境的影响。De Furio还将设计并实施一个专门针对智障儿童和成人的教育项目,利用望远镜和天文馆等普通大学资源。这项工作将利用盖亚天文台提供的地面和空间成像信息,描述两个低密度OB星团、一个高密度结合星团和一个非常年轻的嵌入区域内质量为0.3 M⊙的主星的多样性。有了探测超过10au的伴星的能力,这个项目将:1)探索动力学对多系统形成和保持的影响,2)探索哪种类型的恒星形成区域对银河系场人口有重大贡献,3)对我们对多恒星形成理论的理解作为主质量和轨道分离的函数的基本约束。该奖项反映了美国国家科学基金会的法定使命,并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,被认为值得支持。
英文摘要
Matthew De Furio is awarded an NSF Astronomy and Astrophysics Fellowship to carry out a program of research and education at the University of Texas at Austin. De Furio will observe hundreds of stars within four different star-forming regions (from low-density unbound to high-density bound regions) to identify binary and higher order multiple systems. Results from this work will inform our understanding of the star formation process and explore effects from the stellar birth environment. De Furio will also design and implement an educational program devoted to children and adults with intellectual disabilities using common university resources like telescopes and planetariums.This work will characterize the multiplicity within two low-density OB associations, one high-density bound cluster, and one very young embedded region for primary stars with masses 0.3 M⊙ using ground and space based imaging informed by the Gaia observatory. With the ability to detect companions beyond 10 au, this project will: 1) probe the impact of dynamics on the formation and retention of multiple systems, 2) explore which types of star-forming regions contribute significantly to the Galactic field population, and 3) place fundamental constraints on our understanding of multiple star formation theory as a function of primary mass and orbital separation.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.
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