Tracing the Dynamical States of Intracluster Media (ICMs)

跟踪集群内介质 (ICM) 的动态状态

• 批准号: 1714205
• 负责人: Thomas Jones
• 金额: $ 61.06万
• 依托单位: University of Minnesota-Twin Cities
• 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: 2017-07-01 至 2022-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1714205&HistoricalAwards=false
• 关键词: Tracing; Dynamical; States; Intracluster; Media

The universe has assembled itself by gravity into objects from the size of planets and stars up to galaxies and, on the largest scales, clusters of galaxies. The investigators will focus on understanding the formation of these clusters, giving us important insights into the entire process of how objects form. Galaxy clusters can contain hundreds of galaxies and are filled with very hot gas - their atmospheres, or "intracluster media". These atmospheres are so hot that most of the light they emit is X-rays that can be seen only from space. Astronomers have established that this hot gas has often been highly disturbed when one cluster violently collides and merges with another cluster. The gas motions can tell us about the collisions and how these largest structures in the universe form. Space X-ray telescopes are limited in their abilities to trace these motions, especially outside the denser cluster centers. As it turns out, however, galaxies scattered throughout clusters spew out streams of highly energetic particles that emit radio waves visible from the earth that reveal their interactions with the intracluster media. The intracluster gas motions can also energize radio emitting particles, illuminating the motions. The investigators will find these radio emissions and map their details, using both new and existing ground based radio telescope observations and utilizing the citizen-science-based "Radio Galaxy Zoo." In addition, they will compute detailed physical models to determine how these emissions can be used to trace out the motions of the intracluster media as well as their origins and histories. The results of these studies will substantially improve our understanding of how galaxy clusters form.Galaxy clusters are the largest known gravitationally bound systems in the universe. They are filled with 'intracluster media," diffuse plasmas with temperatures of 10s of millions of degrees, which are visible from space using X-rays. The investigators will address three key questions about these media: 1) what is the dynamical state of the gas, its flows, turbulence and shocks? 2) how do these dynamical features help us understand the cluster formation process? and 3) how do we reliably connect the underlying motions with what we can observe? The investigators will specifically concentrate on behaviors observable at radio wavelengths, using emission from electrons moving at relativistic speeds in the presence of a magnetic field. This allows them to study regimes such as cluster outskirts, for which very little X-ray information is available. They will carry out numerical simulations at the technical frontier, coupling the magnetohydrodynamics of the hot gas to the relativistic particles generating the radio emission. They will conduct new state-of-the-art radio telescope observations and analyses, along with information from the citizen science project Radio Galaxy Zoo on distortions of radio-emitting plasmas caused by the hot gas flows. Together, this work will enable the investigators to gain important information about the cluster formation process, a key piece in the universal picture of how structures in the universe develop over billions of years.

宇宙通过重力将自己组装成从行星和恒星大小到星系，再到最大尺度的星系团的物体。研究人员将专注于了解这些星团的形成，让我们对物体如何形成的整个过程有重要的见解。星系团可以包含数百个星系，充满了非常热的气体--它们的大气层，或“星系团内介质”。这些大气层是如此之热，以至于它们发出的大部分光都是只能从太空中看到的X射线。天文学家已经证实，当一个星系团与另一个星系团猛烈碰撞并合并时，这种高温气体经常受到高度扰动。气体的运动可以告诉我们碰撞以及这些宇宙中最大的结构是如何形成的。空间X射线望远镜追踪这些运动的能力有限，特别是在密度更高的星系团中心之外。然而，事实证明，分散在星系团中的星系喷发出高能粒子流，这些粒子流发出从地球上可见的无线电波，揭示了它们与星系团内介质的相互作用。星系团内的气体运动也可以为射电发射粒子提供能量，从而照亮运动。调查人员将利用新的和现有的地面射电望远镜观测并利用以公民科学为基础的“射电银河动物园”，找到这些射电辐射并绘制其详细信息。此外，他们还将计算详细的物理模型，以确定如何利用这些辐射来追踪星系团内介质的运动以及它们的起源和历史。这些研究的结果将大大提高我们对星系团如何形成的理解。星系团是宇宙中已知的最大的引力约束系统。它们充满了“星系团内介质”，即弥漫的等离子体，温度高达10摄氏度或数百万度，从太空中使用X射线就能看到。研究人员将解决关于这些介质的三个关键问题：1)气体的动力学状态，它的流动，湍流和激波？2)这些动力学特征如何帮助我们理解星系团的形成过程？以及3)我们如何可靠地将潜在的运动与我们所能观察到的联系起来？研究人员将特别关注在无线电波长下可以观察到的行为，使用的是在磁场存在的情况下以相对论速度运动的电子的发射。这使得他们能够研究星系团郊区这样的制度，因为对这些制度来说，X射线信息非常少。他们将在技术前沿进行数值模拟，将热气体的磁流体动力学与产生无线电发射的相对论粒子耦合起来。他们将进行新的最先进的射电望远镜观测和分析，以及公民科学项目无线电银河动物园提供的关于热气流引起的无线电发射等离子体扭曲的信息。总之，这项工作将使研究人员能够获得关于星系团形成过程的重要信息，这是宇宙结构如何在数十亿年内发展的普遍图景中的关键部分。

项目成果

Deep Very Large Array Observations of the Merging Cluster CIZA J2242.8+5301: Continuum and Spectral Imaging

合并星团的深层甚大阵列观测 CIZA J2242.8 5301：连续谱和光谱成像

• DOI: 10.3847/1538-4357/aad738
• 发表时间: 2018
• 期刊: The Astrophysical Journal
• 作者: Gennaro, G. Di;van Weeren, R. J.;Hoeft, M.;Kang, H.;Ryu, D.;Rudnick, L.;Forman, W.;Röttgering, H. J.;Brüggen, M.;Dawson, W. A.
• 通讯作者: Dawson, W. A.

The turbulent pressure support in galaxy clusters revisited

重新审视星系团中的湍流压力支持

• DOI: 10.1093/mnrasl/sly172
• 发表时间: 2018
• 期刊: Monthly Notices of the Royal Astronomical Society: Letters
• 作者: Vazza, F;Angelinelli, M;Jones, T W;Eckert, D;Brüggen, M;Brunetti, G;Gheller, C
• 通讯作者: Gheller, C

The Extraordinary Linear Polarisation Structure of the Southern Centaurus A Lobe Revealed by ASKAP

ASKAP 揭示的南半人马座 A 瓣非凡的线偏振结构

• DOI: 10.3390/galaxies6040127
• 发表时间: 2018
• 期刊: Galaxies
• 影响因子: 2.5
• 作者: Anderson, Craig;Heald, George;O’Sullivan, Shane;Bunton, John;Carretti, Ettore;Chippendale, Aaron;Collier, Jordan;Farnes, Jamie;Gaensler, Bryan;Harvey-Smith, Lisa
• 通讯作者: Harvey-Smith, Lisa

Magnetism Science with the Square Kilometre Array

• DOI: 10.3390/galaxies8030053
• 发表时间: 2020-06
• 期刊: Galaxies
• 影响因子: 2.5
• 作者: G. Heald;S. A. Mao;V. Vacca;T. Akahori;A. Damas-Segovia;B. Gaensler;M. Hoeft;I. Agudo;A. Ba

Chandra and XMM–Newton observations of A2256: cold fronts, merger shocks, and constraint on the IC emission

Chandra 和 XMM-Newton 对 A2256 的观测：冷锋、合并冲击以及对 IC 排放的限制

• DOI: 10.1093/mnras/staa2320
• 发表时间: 2020
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Ge, Chong;Liu, Ruo-Yu;Sun, Ming;Yu, Heng;Rudnick, Lawrence;Eilek, Jean;Owen, Frazer;Dasadia, Sarthak;Rossetti, Mariachiara;Markevitch, Maxim
• 通讯作者: Markevitch, Maxim