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Collaborative Research: Protostellar Jets Across the Mass Spectrum

Collaborative Research: Protostellar Jets Across the Mass Spectrum
合作研究:跨质谱的原恒星喷流
批准号:
1910675
负责人:
Jonathan Tan
金额:
$26.05万
依托单位国家:
美国
项目类别:
Standard Grant
财政年份:
2019
资助国家:
美国
项目状态:
已结题
起止时间:
2019-09-01 至 2023-08-31

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中文摘要
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英文摘要
Stars, like our Sun, are known to form from clouds of molecular gas in interstellar space. These clouds gradually collapse under the influence of gravity, becoming denser and smaller. As this happens, any initial spin of the cloud is amplified, much like when an ice skater pulls their arms in to spin faster. This occurs because of a phenomenon known as the conservation of angular momentum. However, if material that was to form a star fully conserved its angular momentum, i.e., its degree of spin, then by the time it became as small as a star it would be spinning so quickly that it would no longer be stable and would be flung apart. The answer to this riddle of how stars like our Sun have been able to form, requiring quite low rates of spin, is thought to be related to the phenomenon of "Protostellar Jets", which is the subject of this research. Fast flowing gas, collimated into a pair of jets, is almost always seen when young stars are forming, i.e., when they are "protostars". These jets are thought to be launched from a spinning gas disk that surrounds the growing star because of the action of magnetic fields threading the disk that become wound up by the swirling gas. These magnetic fields are thought to become powerful enough to launch some of the gas from the disk, which carries away angular momentum from material left behind that can then eventually settle on to the star. The remnants of such disks may become systems of planets, like those of our solar system. The investigators seek to understand how stars and planets are born by better understanding how protostellar jets are launched. The investigators will perform computer simulations of protostellar jets understand their properties, including from relatively low-mass stars like our Sun, to much more massive stars that also exist in our Galaxy. The results of these simulations will be compared to observations of protostellar jets made by radio telescopes to test the theoretical simulations.The broader impact plan integrates research with teaching and public outreach activities. At the University of the Virgin Islands (UVI) three undergraduates will share in the research projects each year, providing important opportunities for STEM career development for underrepresented groups. This proposal will help strengthen a collaboration between this new research group at UVI and the University of Virginia (UVA). The collaboration plan includes student exchanges between UVI and UVA, expanding the horizons of both groups.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.
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DOI: 10.3847/1538-4357/acbd47
发表时间: 2023-01
期刊: The Astrophysical Journal
影响因子: --
作者: [J. Staff;Kei E. I. Tanaka;J. Ramsey;Yichen Zhang;J. Tan]
通讯作者: J. Staff;Kei E. I. Tanaka;J. Ramsey;Yichen Zhang;J. Tan
Collaborative Research: Peering to the Heart of Massive Star Birth
  • 批准号:
    2206450
  • 项目类别:
    Standard Grant
  • 资助金额:
    $44.95万
  • 财政年份:
    2022
  • 负责人:
    Jonathan Tan
  • 依托单位:
Collaborative Research: Stars from Clouds - Turbulence, Magnetic Fields and Dynamics of Forming Star Clusters
  • 批准号:
    2009674
  • 项目类别:
    Standard Grant
  • 资助金额:
    $29.64万
  • 财政年份:
    2020
  • 负责人:
    Jonathan Tan
  • 依托单位:
Astrophysical and Astrochemical Tests of Massive Star Formation Theories
  • 批准号:
    1819698
  • 项目类别:
    Standard Grant
  • 资助金额:
    $11.57万
  • 财政年份:
    2017
  • 负责人:
    Jonathan Tan
  • 依托单位:
Collaborative Research: Pebbles and Gas - The Supply Chain for Compact Planetary Systems
  • 批准号:
    1834747
  • 项目类别:
    Continuing Grant
  • 资助金额:
    $12.73万
  • 财政年份:
    2017
  • 负责人:
    Jonathan Tan
  • 依托单位:
国内基金
海外基金
Research on Quantum Field Theory without a Lagrangian Description
  • 批准号:
    24ZR1403900
  • 项目类别:
    省市级项目
  • 资助金额:
    --
  • 批准年份:
    2024
  • 负责人:
    SATOSHI NAWATA
  • 依托单位:
Cell Research
Cell Research
Cell Research (细胞研究)