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Collaborative Research: Globular Cluster Formation in Hierarchically Collapsing Clouds as an Origin for Multiple Stellar Populations

合作研究：分层塌缩云中球状星团的形成作为多个恒星族的起源

基本信息

批准号：
1815461
负责人：
Mordecai-Mark Mac Low
金额：
$ 36.7万
依托单位：
American Museum Natural History
依托单位国家：
美国
项目类别：
Standard Grant
财政年份：
2018
资助国家：
美国
起止时间：
2018-08-15 至 2024-07-31
项目状态：
已结题

来源：
https://www.nsf.gov/awardsearch/showAward?AWD_ID=1815461&HistoricalAwards=false
关键词：
Collaborative Research Globular Cluster Formation

项目摘要

Many of the oldest stars ever discovered are found in globular clusters. These are the biggest star clusters known, with millions of stars in a small region. The clusters are fossils of the time early in the history of our universe when stars formed far more often than they do today. The chemical elements that form our planet, and all living beings, were formed during the lives and deaths of such ancient stars. The stars in smaller star clusters are observed to all have almost the same abundances of elements. However, this is not true for globular clusters, which have a spread in abundances. This could give an important clue to how they formed. In the end this will help us to understand our own origins.The investigators will test their new model for how the clusters formed: not as one large cluster, but rather as many smaller clusters that then fell together. Each of the little clusters had its own uniform abundances of elements. When they fell together to make a big cluster, it was a mixture of all the little clusters, so it had a spread of abundances. Observations of globular clusters have recently demonstrated the presence of multiple or spread main sequence populations with varying elemental abundances in virtually every object examined with sufficient care. This is in distinct contrast to less massive open clusters and even observed young massive clusters, which have comparatively uniform elemental abundances. Multiple proposed explanations, which rely on time variability in the star formation rate, contradict current observations.The investigators are developing software tools to model the spread in abundances. These models will run on NSF supercomputers. They will model the gas from which the stars form, and the stars themselves, in separate programs coupled together at every time step. They are building in an adaptive mesh program to model the gas. This innovative method will have many other applications in science and engineering. Their work has broader impacts in the following areas. In education, it will directly support research by a graduate student, and three undergraduates participating in Drexel's exemplary cooperative education program. It will also provide intellectual foundations for the American Museum of Natural History's innovative, residency-based Master of Arts in Teaching Earth (and Space) Science, and for a widely used undergraduate textbook. In outreach, it will provide the foundation for the curation of Hayden Planetarium Space Shows, which are seen by a million visitors a year at the Planetarium, and are licensed to 40 institutions worldwide.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.

迄今为止发现的许多最古老的恒星都是在球状星团中发现的。这些是已知的最大的星星团，在一个小区域内有数百万颗恒星。这些星团是我们宇宙历史早期的化石，那时恒星的形成比今天频繁得多。形成我们星球的化学元素，以及所有生物，都是在这些古老恒星的生命和死亡中形成的。较小的星星星团中的恒星被观察到几乎都有相同的元素丰度。然而，对于球状星团来说，这是不正确的，因为球状星团的丰度是分散的。这可能会为它们如何形成提供重要线索。最后，这将有助于我们理解我们自己的起源。研究人员将测试他们的新模型，以了解星系团是如何形成的：不是一个大星系团，而是许多较小的星系团，然后聚集在一起。每个小星系团都有自己统一的元素丰度。当它们落在一起形成一个大的星团时，它是所有小星团的混合物，所以它有一个丰度的分布。最近对球状星团的观测表明，几乎在每一个仔细检查过的天体中都存在着多个或分散的主序群，它们的元素丰度各不相同。这与质量较小的疏散星团形成鲜明对比，甚至观察到年轻的大质量星团，它们具有相对均匀的元素丰度。多种解释依赖于星星形成速率的时间变化，与目前的观测结果相矛盾。研究人员正在开发软件工具来模拟丰度的传播。这些模型将在NSF超级计算机上运行。他们将模拟恒星形成的气体，以及恒星本身，在每个时间步耦合在一起的单独程序中。他们正在建立一个自适应网格程序来模拟气体。这种创新的方法将在科学和工程中有许多其他应用。他们的工作在以下领域产生了广泛的影响。在教育方面，它将直接支持一名研究生和三名本科生参加德雷克塞尔大学的示范性合作教育计划的研究。它还将为美国自然历史博物馆的创新，以居住为基础的地球（和空间）科学教学艺术硕士和广泛使用的本科教科书提供知识基础。在推广方面，它将为海登天文馆太空展的策展提供基础，每年有100万游客在天文馆观看，并授权给全球40个机构。该奖项反映了NSF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。

项目成果

期刊论文数量（31）

专著数量（0）

科研奖励数量（0）

会议论文数量（0）

专利数量（0）

How do velocity structure functions trace gas dynamics in simulated molecular clouds?

速度结构函数如何追踪模拟分子云中的气体动力学？

DOI：
10.1051/0004-6361/201833970
发表时间：
2019
期刊：
Astronomy & Astrophysics
影响因子：
6.5
作者：
Chira, R.-A.;Ibáñez-Mejía, J. C.;Mac Low, M.-M.;Henning, Th.
通讯作者：
Henning, Th.

The Small-scale Dynamo in a Multiphase Supernova-driven Medium

多相超新星驱动介质中的小型发电机

DOI：
10.3847/1538-4357/acac20
发表时间：
2023
期刊：
The Astrophysical Journal
影响因子：
0
作者：
Gent, Frederick A.;Mac Low, Mordecai-Mark;Korpi-Lagg, Maarit J.;Singh, Nishant K.
通讯作者：
Singh, Nishant K.

Simulations of the star-forming molecular gas in an interacting M51-like galaxy

对相互作用的类 M51 星系中恒星形成分子气体的模拟

DOI：
10.1093/mnras/stz3600
发表时间：
2020
期刊：
Monthly Notices of the Royal Astronomical Society
影响因子：
4.8
作者：
Tress, Robin G.;Smith, Rowan J.;Sormani, Mattia C.;Glover, Simon C. O.;Klessen, Ralf S.;Mac Low, Mordecai-Mark;Clark, Paul C.
通讯作者：
Clark, Paul C.

Symmetry Breaking in Dynamical Encounters in the Disks of Active Galactic Nuclei

DOI：
10.3847/2041-8213/ac400a
发表时间：
2021-10
期刊：
The Astrophysical Journal Letters
影响因子：
0
作者：
Yihan Wang;B. McKernan;Saavik Ford;R. Perna;N. Leigh;M. M. Low-M.
通讯作者：
Yihan Wang;B. McKernan;Saavik Ford;R. Perna;N. Leigh;M. M. Low-M.

Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes. II. Spins and Incoming Objects

DOI：
10.3847/1538-4357/abbc1d
发表时间：
2018-07
期刊：
The Astrophysical Journal
影响因子：
0
作者：
Amy Secunda;J. Bellovary;M. Mac Low;K. Ford;B. McKernan;N. W. C. Leigh;W. Lyra;Z. Sándor;J. A
通讯作者：
Amy Secunda;J. Bellovary;M. Mac Low;K. Ford;B. McKernan;N. W. C. Leigh;W. Lyra;Z. Sándor;J. A