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Feeding and Feedback: Understanding the Assembly of Galactic Disks

Feeding and Feedback: Understanding the Assembly of Galactic Disks
馈送和反馈:了解银河盘的组装
批准号:
1817125
负责人:
Crystal Martin
金额:
$50.56万
依托单位国家:
美国
项目类别:
Continuing Grant
财政年份:
2018
资助国家:
美国
项目状态:
已结题
起止时间:
2018-08-31 至 2023-08-31

项目摘要

项目成果

Crystal Martin的其他基金

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中文摘要
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英文摘要
The growth of galaxies occurs as the galaxies gather gas from their surroundings to produce stars. The stars will then produce a 'wind' that is driven by starlight and energetic particles along with supernovae from the explosion of more massive stars. This wind serves to drive gas away from the galaxies which slows down the star formation rate. This project will study the flow of gas in and out of star forming galaxies by looking at how the light from distant quasars is absorbed as it passes through the gas surrounding the more nearby star forming galaxies. The project will also compare their results with cosmological simulations to better understand both the simulations and the status of the galaxies. The project will also enhance the educational opportunities for underrepresented minorities from elementary school to the graduate level.As galaxies grow, they accrete gas from their surroundings to feed their star formation. As they form stars, they produce a galactic wind that drives gas away. This project will study the flow of gas in and out of star forming galaxies. The flow of the gas will be measured by observing absorption lines from circum-galactic gas lying along the line-of-sight to distant quasars. This will give us a better understanding of how gas flows in and out of galaxies as they grow. The project will analyze 50 new sightlines, sampling the circum-galactic medium (CGM) around several typical star forming galaxies. The project will then compare these results with cosmological simulations of galaxy formation, using the EAGLE simulations. The project will also perform a ?Look Back Study? by comparing galaxies at redshifts of ~0.2 with their lower mass progenitors a redshifts of 2. In this part, the project will look at clumpy distant galaxies and statistically determine if the clumpiness can be related to different outflows of gas. The project will also enhance the educational opportunities for underrepresented minorities from elementary school to the graduate level.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.
期刊论文(15)
专著(0)
科研奖励(0)
会议论文
DOI: 10.3847/1538-4357/ab0ec2
发表时间: 2019-03
期刊: The Astrophysical Journal
影响因子: --
作者: [S. Ho;C. Martin;M. Turner]
通讯作者: S. Ho;C. Martin;M. Turner
Resolving 3D Disk Orientation Using High-resolution Images: New Constraints on Circumgalactic Gas Inflows
使用高分辨率图像解析 3D 圆盘方向:环银河系气体流入的新限制
DOI: 10.3847/1538-4357/ab58cd
发表时间: 2020
期刊: The Astrophysical Journal
影响因子: --
作者: [Ho, Stephanie H., Martin, Crystal L.]
通讯作者: Martin, Crystal L.
How Identifying Circumgalactic Gas by Line-of-sight Velocity instead of the Location in 3D Space Affects O vi Measurements
通过视线速度而不是 3D 空间中的位置来识别绕银河系气体如何影响 O vi 测量
DOI: 10.3847/1538-4357/ac2c73
发表时间: 2021
期刊: The Astrophysical Journal
影响因子: --
作者: [Ho, Stephanie H., Martin, Crystal L., Schaye, Joop]
通讯作者: Schaye, Joop
DOI: 10.3847/1538-4357/ac1105
发表时间: 2021-07
期刊: The Astrophysical Journal
影响因子: --
作者: [A. Henry;M. Rafelski;B. Sunnquist;N. Pirzkal;C. Pacifici;H. Atek;M. Bagley;I. Baronchelli;G. Barro;A. Bunker;J. Colbert;Y. Dai;B. Elmegreen;D. Elmegreen;S. Finkelstein;D. Kocevski;A. Koekemoer;M. Malkan;C. Martin;V. Mehta;A. Pahl;C. Papovich;M. Rutkowski;J. Sánchez Almeida;C. Scarlata;G. Snyder;H. Teplitz]
通讯作者: A. Henry;M. Rafelski;B. Sunnquist;N. Pirzkal;C. Pacifici;H. Atek;M. Bagley;I. Baronchelli;G. Barro;A. Bunker;J. Colbert;Y. Dai;B. Elmegreen;D. Elmegreen;S. Finkelstein;D. Kocevski;A. Koekemoer;M. Malkan;C. Martin;V. Mehta;A. Pahl;C. Papovich;M. Rutkowski;J. Sánchez Almeida;C. Scarlata;G. Snyder;H. Teplitz
13
    Evolution of Circumgalactic Gas Flows
    Empirical Calibration of Feedback Processes in Galaxy Evolution
    国内基金
    海外基金
    Dynamic Credit Rating with Feedback Effects
    • 批准号:
      --
    • 项目类别:
      外国学者研究基金项目
    • 资助金额:
      --
    • 批准年份:
      2024
    • 负责人:
      Christian Martin Hilpert
    • 依托单位: