New CO(1-0) Survey of Nearby Galaxies: Evolution of Molecular Gas and Star Formation in Galactic Disks

对附近星系的新 CO(1-0) 巡天：星系盘中分子气体的演化和恒星形成

• 批准号: 1211680
• 负责人: Jin Koda
• 金额: $ 42.42万
• 依托单位: SUNY at Stony Brook
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2012
• 资助国家: 美国
• 起止时间: 2012-07-01 至 2017-06-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1211680&HistoricalAwards=false
• 关键词: New; CO; Survey; Nearby; Galaxies

A longstanding problem in astrophysics is to understand how galaxies form and develop throughout their lifetimes. Such understanding is necessary to uncover how our Universe evolved and to gain insight into the origin of our own Milky Way Galaxy. One important aspect of understanding galaxy formation and evolution is to develop detailed theories of star formation. As star formation occurs in giant molecular clouds (GMCs) within galaxies, astrophysicists study the formation and evolution of GMCs. With unprecedented high quality and high resolution data, this study will explore the evolution of GMCs and consequent star formation in galactic disks, and it will critically and quantitatively reconsider the standard picture of gas evolution in galaxies, specifically the one driven by stellar feedback. The study enables for the first time a census of GMC populations in substantial spiral galaxies.This project will also serve as a prototype for research with the Atacama Large Millimeter/submillimeter Array (ALMA) (a new international facility funded in part by the National Science Foundation), which will resolve the internal structure of GMCs in nearby galaxies and routinely produce images of molecular gas and star formation in very distant galaxies. For this project the investigators will use observations from their new CO survey of nearby galaxies with the Combined Array for Research in Millimeter-wave Astronomy (CARMA) and the Nobeyama Radio Observatory 45m telescope (NRO45), a survey that is nearly complete. The investigators will release to the astronomical community the CO data of nearby galaxies from CARMA and NRO45, and they will also release the software for the combination of interferometer and single-dish data developed for the survey.The investigating team also plans educational and outreach activities that involve building a radio interferometer for a hands-on astronomical laboratory course and disseminating the course materials to other schools. Because the concept of interferometry is challenging to master, developing such a hands-on laboratory course is crucial to the education of the next generation of radio astronomers for the ALMA era.

天体物理学的一个长期问题是了解星系在其一生中是如何形成和发展的。 这样的理解对于揭示我们的宇宙是如何演化的以及深入了解我们银河系的起源是必要的。 理解星系形成和演化的一个重要方面是发展详细的星星形成理论。 由于星系内的巨分子云（GMC）中存在星星的形成过程，天体物理学家对GMC的形成和演化进行了研究。 本研究将以前所未有的高质量和高分辨率数据，探索星系盘中GMC的演化和随后的星星形成，并将批判性地和定量地重新考虑星系气体演化的标准图像，特别是恒星反馈驱动的图像。 该研究首次实现了对大量螺旋星系中GMC种群的普查。该项目也将作为阿塔卡马大型毫米/亚毫米阵列（阿尔马）研究的原型。（一个新的国际设施，部分由国家科学基金会资助），它将解析附近星系中GMC的内部结构，并定期生成非常遥远的分子气体和星星形成的图像。星系 对于这个项目，研究人员将使用他们新的CO调查的观测结果，该调查使用毫米波天文学研究组合阵列（CARMA）和Nobeyama射电天文台45米望远镜（NRO 45），该调查已接近完成。 研究人员将向天文学界发布CARMA和NRO 45的邻近星系CO数据，他们还将发布为调查开发的干涉仪和单碟数据组合软件。调查小组还计划开展教育和推广活动，包括建造射电干涉仪，用于天文实验室实践课程，并将课程材料分发给其他学校。 由于干涉测量的概念是具有挑战性的掌握，开发这样一个动手实验室课程是至关重要的阿尔马时代的下一代射电天文学家的教育。