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RUI: Chemical Abundances of Galactic Compact Planetary Nebulae

RUI: Chemical Abundances of Galactic Compact Planetary Nebulae
RUI:银河致密行星状星云的化学丰度
批准号:
1616807
负责人:
Ting-Hui Lee
金额:
$12.78万
依托单位国家:
美国
项目类别:
Standard Grant
财政年份:
2016
资助国家:
美国
项目状态:
已结题
起止时间:
2016-07-15 至 2021-06-30

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中文摘要
翻译
研究人员研究了我们银河系恒星中产生的元素。所有恒星都通过将轻元素融合成较重的元素在其核心产生能量。当恒星的核心没有轻元素可聚变时,它会在自身重量的作用下收缩。坍塌重新加热了外层,将这颗恒星变成了一颗红巨星。这个阶段是不稳定的,以外层被完全抛出而结束。这些元素是在恒星生命周期结束时释放出来的。研究人员将使用光学望远镜测量元素丰度。这些元素可以在行星状星云中看到,行星状星云是由这样的恒星抛出的美丽的电离气态外壳。本科生将帮助进行这项研究。研究人员将向学生介绍科学和工程研究的技术。从恒星产生的元素的图像中,研究人员了解这些恒星中发生的核反应的类型。从这些反应中,研究人员了解了这些恒星的质量和寿命。有些元素原封不动地穿过恒星的核火。通过匹配这些元素,他们可以追踪恒星诞生的分子云的类型。使用高精度的行星状星云的光学和红外光谱与更新、更精确的距离测量相结合的新方法,他们将研究整个银河系恒星形成和化学浓缩的历史。西肯塔基大学的本科生将在这项工作的各个方面发挥积极作用。学生们将为在科学和技术领域的职业生涯做好更好的准备。这名调查员在该国最需要此类工作的地区工作。
英文摘要
The investigators study the elements produced in stars in our galaxy. All stars generate energy in their cores by fusing light elements into heavier ones. When the core of a star runs out of light elements to fuse, its contracts under its own weight. The collapse reheats the outer layers, turning the star into a red giant. This phase is unstable and ends with the outer layers being thrown off entirely. These elements are released from the stars at the end of their life cycle. The investigators will use optical telescopes to measure the element abundances. The elements are visible in planetary nebulae, which are beautiful ionized gaseous shells ejected by such stars. Undergraduate students will help with the research. The students will be introduced to the techniques of scientific and engineering research.From images of the elements created by the stars, the investigators learn the types of nuclear reactions that went on in these stars. From the reactions, the investigator learns how massive the stars were and how long they lived. Some elements pass through the star's nuclear fires unchanged. By matching these elements, they can trace the type of molecular clouds where the stars were born. Using new methods combining high-precision optical and infrared spectra of planetary nebulae with newer, more accurate distance measurements, they will examine the history of star formation and chemical enrichment throughout our Galaxy. Undergraduate students at Western Kentucky University will take active roles in all aspects of this work. The students will become better prepared for careers in scientific and technical fields. The investigator is working in a region of the country where such jobs are most needed.
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Chinese Journal of Chemical Engineering
  • 批准号:
    21224004
  • 项目类别:
    专项基金项目
  • 资助金额:
    20.0万元
  • 批准年份:
    2012
  • 负责人:
    廖叶华
  • 依托单位:
Chinese Journal of Chemical Engineering
  • 批准号:
    21024805
  • 项目类别:
    专项基金项目
  • 资助金额:
    20.0万元
  • 批准年份:
    2010
  • 负责人:
    廖叶华
  • 依托单位: