Consolidated Grant Astronomy Observation and Theory 2022-2025

综合格兰特天文学观测和理论 2022-2025

• 批准号: ST/W000997/1
• 负责人: Richard McMahon
• 金额: $ 221.32万
• 依托单位: University of Cambridge
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2022
• 资助国家: 英国
• 起止时间: 2022 至 无数据
• 项目状态: 未结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FW000997%2F1
• 关键词: Consolidated; Grant; Astronomy; Observation; Theory

This consolidated grant proposal is to support leading research in theoretical and observational astronomy at the Institute of Astronomy (IoA), University of Cambridge.On the largest scales, the proposal includes work to understand the origin and evolution of the Universe itself through analysis of precise observations of the cosmic microwave background with new ground-based telescopes, and signals from neutral hydrogen probing the era of cosmic dawn, when the first generation of stars and black holes reheated and reionized the cold and neutral post-recombination Universe, bringing the cosmic dark ages to an end. The Universe today is filled with galaxies, of which our own Milky Way is a not atypical example. A full understanding of galaxy formation and evolution requires multiple lines of attack. Observations of the resolved stellar populations in the Milky Way and its Local Group companions provide a detailed fossil record of the dynamical assemblies of the galaxies, the formation of stars, and the buildup of heavy elements over a wide range of mass scales and initial conditions. Researchers at the IoA lead key parts of the data processing for the ESA Gaia space mission, which is performing a survey of the Milky Way with unprecedented precision and volume. Several projects in this proposal will exploit the forthcoming third data release from Gaia to understand the dynamics of the Galaxy and its companions. At the other end of the scale, observations of distant galaxies spanning lookback times of up to 12 billion years provide direct measurements of the evolution of galaxy populations and the buildup of stars and metals with cosmic time. The light from these first galaxies likely led to the reionization of hydrogen in the intergalactic medium, when the age of the Universe was less than one billion years. Modelling this process requires sophisticated hydrodynamical simulations, including radiative transfer effects, and is a further focus of this proposal.It is now recognised that there is an intimate link between the evolution of galaxies and the origin and properties of super-massive black holes, which reside at the centre of the Milky Way and other galaxies. The regions close to black holes allow the exploration of physics at the extremes. The formation and properties of super-massive black holes and their relation to the galaxies will be explored in this grant with sophisticated computational simulations of merging galaxies.On much smaller scales within galaxies, the grant focusses of the formation of planetary systems through theoretical modelling of the evolution of protoplanetary disks (exploiting high-resolution imaging with ALMA) and their associated debris disks, and on the atmospheres and geology of extrasolar planets.

这项综合拨款提案将支持剑桥大学天文学研究所（IoA）在理论和观测天文学方面的领先研究。在最大尺度上，该提案包括通过分析新的地面望远镜对宇宙微波背景的精确观测来了解宇宙本身的起源和演化，以及来自中性氢探测宇宙黎明时代的信号，当第一代恒星和黑洞重新加热和重新电离冷和中性后复合宇宙，使宇宙黑暗时代结束。今天的宇宙充满了星系，我们自己的银河系就是一个不典型的例子。要全面了解星系的形成和演化，需要多方面的研究。对银河系和它的本星系群伴星的观测提供了详细的化石记录，记录了星系的动力学组装、恒星的形成以及在广泛的质量尺度和初始条件下重元素的积累。IoA的研究人员领导了欧空局盖亚空间使命数据处理的关键部分，该任务正在以前所未有的精度和数量对银河系进行调查。该提案中的几个项目将利用盖亚即将发布的第三次数据来了解银河系及其同伴的动力学。在尺度的另一端，对遥远星系的观测跨越了长达120亿年的回望时间，提供了对星系种群演化以及恒星和金属随宇宙时间的积累的直接测量。来自这些第一个星系的光可能导致星系际介质中氢的再电离，当时宇宙的年龄不到10亿年。模拟这一过程需要复杂的流体动力学模拟，包括辐射传输效应，这也是本提案的进一步重点。现在人们认识到，星系的演化与位于银河系和其他星系中心的超大质量黑洞的起源和性质之间存在着密切的联系。接近黑洞的区域允许在极端情况下探索物理学。本研究金将透过复杂的星系合并计算模拟，探讨超大质量黑洞的形成和性质，以及它们与星系的关系。本研究金的重点是透过原行星盘演化的理论模拟，研究星系内更小尺度的行星系统的形成（利用阿尔马的高分辨率成像）及其相关的碎片盘，以及太阳系外行星的大气和地质。

项目成果

Accretion rates in hierarchical triple systems with discs

带圆盘的分层三重系统中的吸积率

• DOI: 10.17863/cam.107323
• 发表时间: 2022
• 作者: Ceppi S

Secondary gas in debris discs released following the decay of long-lived radioactive nuclides, catastrophic, or resurfacing collisions

长寿命放射性核素衰变、灾难性或重铺碰撞后碎片盘中释放的二次气体

• DOI: 10.1093/mnras/stad2912
• 发表时间: 2023
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Bonsor A

The clumpy structure of ? Eridani's debris disc revisited by ALMA

的块状结构？

• DOI: 10.1093/mnras/stad938
• 发表时间: 2023
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Booth M

Azimuthal temperature variations in ISO-Oph 2 from multifrequency ALMA observations

多频 ALMA 观测中 ISO-Oph 2 的方位角温度变化

• DOI: 10.1093/mnras/stad1981
• 发表时间: 2023
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Casassus S

An ALMA Survey of M-dwarfs in the Beta Pictoris Moving Group with two new debris disc detections

ALMA 对绘架座移动群中的 M 矮星进行的巡天，发现了两个新的碎片盘

• DOI: 10.1093/mnras/stad3083
• 发表时间: 2023
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Cronin-Coltsmann P