Galaxy interactions in groups and clusters behind the Magellanic Clouds

麦哲伦云后面的星系群和星团中的星系相互作用

• 批准号: 2482940
• 金额: --
• 依托单位: Keele University
• 依托单位国家: 英国
• 项目类别: Studentship
• 财政年份: 2020
• 资助国家: 英国
• 起止时间: 2020 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=studentship-2482940
• 关键词: Galaxy; interactions; groups; clusters; behind

This research project aims to, first, identify groups and clusters of galaxies behind the Magellanic Clouds and, then, characterise galaxy interactions and their effects on the galaxies' morphology, star formation rate and nuclear activity as a function of environment and redshift. Two main types of interaction will form part of this assessment: galaxy-galaxy and galaxy-ICM (Intra-Cluster Medium). The analysis will be based on recently completed multi-wavelength imaging surveys and associated source catalogues, and the application of automated and/or machine learning algorithms. Followup observational programmes will be designed in order to test methodologies and gain detailed insight.

该研究项目的目的是首先确定麦哲伦云背后的星系组和簇，然后以星系相互作用及其对星系的形态，星形形成率和核活动的影响来表征环境和红移的函数。两种主要的相互作用将构成此评估的一部分：星系 - 果岭和Galaxy-ICM（集群内培养基）。该分析将基于最近完成的多波长成像调查和相关的源目录，以及自动化和/或机器学习算法的应用。将设计后续观察程序，以测试方法论并获得详细的见解。

项目成果

The VMC survey - XLIX. Discovery of a population of quasars dominated by nuclear dust emission behind the Magellanic Clouds

VMC 调查 - XLIX。

• DOI: 10.1093/mnras/stac2096
• 发表时间: 2022
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Pennock C