Collaborative Research: A Quantitative Framework for the Flow of Metals in Nearby Galaxies

合作研究：邻近星系金属流动的定量框架

• 批准号: 1806926
• 负责人: Kristen McQuinn
• 金额: $ 25.56万
• 依托单位: University of Texas at Austin
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2018
• 资助国家: 美国
• 起止时间: 2018-08-15 至 2019-09-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1806926&HistoricalAwards=false
• 关键词: Collaborative; Research; Quantitative; Framework; Flow

Chemical elements, such as oxygen and nitrogen, are forged in the interior of stars. When stars end their lives as supernova explosions, many of these elements are expelled and mix into the local environment within a galaxy. These expelled elements are the seeds for future generations of stars and planets. If there are enough supernova explosions, or if the galaxy is small, some of the elements will leave the galaxy entirely and end up in intergalactic space. Therefore, measuring the types of elements in galaxies, and finding where the elements are located, give important clues about the history of galaxies in the Universe. These investigators will perform optical and radio wavelength observations of 36 nearby galaxies to study how galaxies produce, distribute, and expel elements. Their research results will help us understand how galaxies change over time and will be used as input to galaxy formation models. Fundamentally, the observed gas-phase metallicities in nearby galaxies should correspond to the production and release of stellar nucleosynthesis products and, thus, provide a robust trace of galaxy formation and life cycle. Global scaling relations, such as the mass-metallicity relation, show gas-phase metallicities increase steeply with galaxy mass. The investigators seek to build an over-arching, quantitative framework of the production, transport, distribution, and retention of metals in low-mass galaxies. Specifically, they will determine the full chemical enrichment histories of a statistical sample of low-mass galaxies in the nearby universe from a comprehensive set of spectroscopic and imaging data.The investigators, both women astronomers, will work to develop a diverse, globally competitive STEM workforce by working with undergraduate and graduate students on this research project. Additionally, their research highlights will be broadcasted on the public "StarDate" Radio program to an audience of 750,000. The co-investigator will continue to lead nationwide efforts to reduce interference at radio wavelengths. The efforts to reduce radio interference are critical for enabling radio astronomy research.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

化学元素，如氧和氮，在恒星内部形成。当恒星以超新星爆炸结束生命时，许多这些元素被驱逐并混合到星系内的局部环境中。这些被驱逐的元素是未来恒星和行星的种子。如果有足够多的超新星爆炸，或者星系很小，一些元素将完全离开星系，最终进入星系际空间。因此，测量星系中元素的类型，并找到元素的位置，可以为宇宙中星系的历史提供重要线索。 这些研究人员将对36个邻近星系进行光学和无线电波长观测，以研究星系如何产生，分布和排出元素。他们的研究结果将帮助我们了解星系如何随着时间的推移而变化，并将被用作星系形成模型的输入。从根本上说，在附近星系中观测到的气相金属丰度应该与恒星核合成产物的产生和释放相对应，从而提供了星系形成和生命周期的有力线索。全球尺度关系，如质量-金属丰度关系，显示气相金属丰度随星系质量急剧增加。研究人员试图建立一个过度的，定量的框架的生产，运输，分布和保留的金属在低质量星系。 具体来说，他们将从一套全面的光谱和成像数据中确定附近宇宙中低质量星系统计样本的完整化学富集历史。两位女天文学家将通过与本科生和研究生合作开展这一研究项目，努力培养一支多元化、具有全球竞争力的STEM队伍。 此外，他们的研究重点将在公共“StarDate”电台节目中播出，听众人数为75万。共同调查员将继续领导全国努力减少无线电波段的干扰。 减少无线电干扰的努力对射电天文学研究至关重要。该奖项反映了NSF的法定使命，并通过使用基金会的知识价值和更广泛的影响审查标准进行评估，被认为值得支持。