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THE MAGELLANIC STREAM: AGING, EXTENSION, AND ORBITS OF THE MAGELLANIC CLOUDS

THE MAGELLANIC STREAM: AGING, EXTENSION, AND ORBITS OF THE MAGELLANIC CLOUDS
麦哲伦流:麦哲伦云的老化、延伸和轨道
批准号:
0908134
负责人:
Snezana Stanimirovic
金额:
$18.27万
依托单位国家:
美国
项目类别:
Standard Grant
财政年份:
2009
资助国家:
美国
项目状态:
已结题
起止时间:
2009-09-01 至 2012-08-31

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中文摘要
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英文摘要
This award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5). Under this award, Dr. Snezana Stanimirovic (University of Wisconsin - Madison) will carry out a study of how the hot Galactic atmosphere shapes the evolution of the Magellanic Stream (MS), a spectacular 100-degree long tail of neutral hydrogen (HI) trailing behind our closest neighbors, the Magellanic Clouds (MCs). This study is motivated by the recent discovery of a significant extension and of the complexity of MS gas. The complex small-scale structure of the MS gas suggests that dynamic interactions with the hot Galactic atmosphere are at work, especially at the northern extension of the MS. This area, in the form of several long filaments, is not explained by traditional models of the interactions between the Galaxy and the MCs. This project will obtain the most sensitive radio and optical observations to date of several regions along the MS with the Arecibo and Green Bank radio telescopes, and the Wisconsin-Indiana-Yale-National Optical Astronomy Observatory optical telescopes. The deep observations to be made will be used to search for morphological and spectral signatures of interactions between the Galactic atmosphere and the MS. The observations are essential samples to assess the prevalence and importance of different types of instabilities in the interface regions where these two media meet.This research will be the core topic of a Ph.D. dissertation at the University of Wisconsin-Madison and, therefore, represents a focused confluence of research and education. Another aspect of this project will be a collaboration with the staff at the Arecibo radio telescope to design and integrate a new method for the suppression of a strong radio interference signal caused by the Global Positioning System, which obliterates astronomical observations at a frequency of 1381 Megahertz. The developed method will be applicable to all radio telescopes world-wide. In addition, a new-generation education and research facility, based on three small radio telescopes, will be developed at the University of Wisconsin to integrate research with undergraduate classes.
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Collaborative Research: Charting the Supernova-Gas-Stars Connection via a Major New VLA Survey of the Local Group
  • 批准号:
    2205630
  • 项目类别:
    Standard Grant
  • 资助金额:
    $13.74万
  • 财政年份:
    2022
  • 负责人:
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  • 依托单位:
How does stellar feedback drive interstellar turbulence and molecular hydrogen formation?
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    2108370
  • 项目类别:
    Standard Grant
  • 资助金额:
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  • 财政年份:
    2021
  • 负责人:
    Snezana Stanimirovic
  • 依托单位:
CAREER: Diffuse interstellar clouds as the key step in galaxy evolution
  • 批准号:
    1056780
  • 项目类别:
    Continuing Grant
  • 资助金额:
    $80.68万
  • 财政年份:
    2011
  • 负责人:
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REU Site for Astronomy and Astrophysics at UW-Madison: 2010 and beyond
  • 批准号:
    1004881
  • 项目类别:
    Continuing Grant
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  • 财政年份:
    2010
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  • 依托单位:
国内基金
海外基金
基于LAMOST和GAIA的Magellanic Stream化学-动力学研究
  • 批准号:
    11773033
  • 项目类别:
    面上项目
  • 资助金额:
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  • 批准年份:
    2017
  • 负责人:
    张岚
  • 依托单位: