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Radio Continuum Observations of Active Stars

Radio Continuum Observations of Active Stars
活跃恒星的射电连续体观测
批准号:
9217891
负责人:
Stephen White
金额:
$13.2万
依托单位国家:
美国
项目类别:
Continuing Grant
财政年份:
1993
资助国家:
美国
项目状态:
已结题
起止时间:
1993-02-01 至 1997-01-31

项目摘要

项目成果

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中文摘要
翻译
利用VLA改进的灵敏度,现在可以探测和研究来自恒星日冕的射电辐射。PI正在利用这种能力来调查各种已知或预计会有日冕的恒星。这些包括弱线T Tau星,dMe耀斑星,RS CVn双星,在。英仙座星团,快速旋转的K矮星AB Dor等等。目的是了解日冕的结构和潜在的物理过程。
英文摘要
It is now possible to detect and study radio emission from the coronae of stars by using the improved sensitivity of the VLA. The PI is exploiting this capability to survey a variety of stars which are known or expected to have coronae. These include weak-lined T Tau stars, dMe flare stars, RS CVn binaries, stars in the . Persei cluster, the rapidly rotating K dwarf AB Dor, etc. The goal is to understand the structure and underlying physical processes of the coronae.
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