Modeling the Formation of Disks of Gas and Dust Around Young Stars

模拟年轻恒星周围气体和尘埃盘的形成

• 批准号: 1716259
• 负责人: Zhi-Yun Li
• 金额: $ 35.34万
• 依托单位: University of Virginia Main Campus
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2017
• 资助国家: 美国
• 起止时间: 2017-09-01 至 2022-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1716259&HistoricalAwards=false
• 关键词: Modeling; Formation; Disks; Gas; Dust

This astronomy project will use computer models to understand how disks of gas and dust form around very young stars. It is from these disks that planets, like Earth and the other planets in our Solar System, are formed. There is now strong evidence that most, if not all, stars in our Galaxy have their own system of planets. The team at the University of Virginia will use sophisticated computer code that they have been working with for many years to study this process. They will include the effects of "magnetic fields" and "turbulence" in their models. Both are thought to be important processes in space, especially in the large clouds that we know lie between the stars. These clouds collapse under their own weight to form stars and planets. A graduate and an undergraduate student will be involved in this project. The investigators will produce animated movies of disk formation for use in large introductory astronomy classes for non-science majors and will develop activities for a mobile planetarium as part of the "Dark Skies, Bright Kids" program, a science educational activity that targets elementary school students in rural Albemarle County, Virginia.Star-forming cores are observed to be significantly magnetized and magnetic braking has been shown to be capable of suppressing disk formation, leading to the so-called magnetic braking catastrophe. The goal of the proposed program is to determine whether the two leading candidates for averting the catastrophe, non-ideal magnetohydrodynamic (MHD) effects and turbulence, can allow the planet-forming disks to form in the presence of a realistic magnetic field, and whether such disks satisfy the increasingly tight observational constraints set by recent ALMA observations. The proposers will use and further develop a well-tested MHD code known as ZeusTW. In the second part of the project they will use the ENZO adaptive mesh refinement MHD code to synthesize disk formation in isolated cores and in clusters.

这个天文学项目将使用计算机模型来了解年轻恒星周围的气体和灰尘盘如何形成。 正是从这些磁盘中形成了像地球和太阳系中其他行星一样的行星。 现在有强有力的证据表明，我们银河系中的大多数（如果不是全部）的明星都有自己的行星系统。 弗吉尼亚大学的团队将使用他们多年来一直在研究此过程的复杂计算机代码。 它们将在其模型中包括“磁场”和“湍流”的效果。 两者都被认为是太空中的重要过程，尤其是在我们所知道的大云层中。 这些云在自己的重量下崩溃，形成恒星和行星。 毕业生和本科生将参与该项目。 调查人员将制作动画电影的磁盘形成电影，以用于非科学专业的大型入门天文学课程，并将为“黑暗的天空，明亮的孩子”计划的一部分开发移动人工界的活动，该计划是针对科学教育活动的一项科学教育活动，科学教育活动是弗吉尼亚州阿尔巴尔县农村地区的小学生。所谓的磁制动灾难。拟议程序的目的是确定两个领先的候选者避免灾难，非理想的磁性水力动力学（MHD）效果和湍流是否可以使行星形成的磁盘在存在逼真的磁场的情况下形成，以及该磁盘是否满足了越来越严格的严格的观察障碍，该磁盘是否满足了最近的高度观察构造的测量。 提议者将使用并进一步开发经过良好测试的MHD代码，称为Zeustw。 在项目的第二部分中，他们将使用ENZO自适应网格改进MHD代码来合成隔离核心和簇中的磁盘形成。

项目成果

ALMA Dust Polarization Observations of Two Young Edge-on Protostellar Disks

两个年轻的边缘原恒星盘的 ALMA 尘埃偏振观测

• DOI: 10.3847/1538-4357/aaa769
• 发表时间: 2018
• 期刊: The Astrophysical Journal
• 作者: Lee, Chin-Fei;Li, Zhi-Yun;Ching, Tao-Chung;Lai, Shih-Ping;Yang, Haifeng
• 通讯作者: Yang, Haifeng

Does HL Tau disc polarization in ALMA band 3 come from radiatively aligned grains?

ALMA 带 3 中的 HL Tau 圆盘极化是否来自辐射排列的颗粒？

• DOI: 10.1093/mnras/sty3263
• 发表时间: 2018
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Yang, Haifeng;Li, Zhi-Yun;Stephens, Ian W;Kataoka, Akimasa;Looney, Leslie
• 通讯作者: Looney, Leslie

Validating scattering-induced (sub)millimetre disc polarization through the spectral index, wavelength-dependent polarization pattern, and polarization spectrum: the case of HD 163296

• DOI: 10.1093/mnras/staa1499
• 发表时间: 2019-12
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Zheyu Lin;Zhi-Yun Li;Haifeng Yang;L. Looney;I. Stephens;C. Hull

Kinematic Analysis of a Protostellar Multiple System: Measuring the Protostar Masses and Assessing Gravitational Instability in the Disks of L1448 IRS3B and L1448 IRS3A

原恒星多重系统的运动学分析：测量原恒星质量并评估 L1448 IRS3B 和 L1448 IRS3A 盘中的引力不稳定性

• DOI: 10.3847/2041-8213/abcc02
• 发表时间: 2021
• 期刊: The Astrophysical Journal Letters
• 作者: Reynolds, Nickalas K.;Tobin, John J.;Sheehan, Patrick;Sadavoy, Sarah I.;Kratter, Kaitlin M.;Li, Zhi-Yun;Chandler, Claire J.;Segura-Cox, Dominique;Looney, Leslie W.;Dunham, Michael M.
• 通讯作者: Dunham, Michael M.

Relative alignment between dense molecular cores and ambient magnetic field: the synergy of numerical models and observations

致密分子核心和环境磁场之间的相对排列：数值模型和观测的协同作用

• DOI: 10.1093/mnras/staa835
• 发表时间: 2020
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Chen, Che-Yu;Behrens, Erica A;Washington, Jasmin E;Fissel, Laura M;Friesen, Rachel K;Li, Zhi-Yun;Pineda, Jaime E;Ginsburg, Adam;Kirk, Helen;Scibelli, Samantha
• 通讯作者: Scibelli, Samantha