Molecules and dust around AGB stars
Molecules and dust around AGB stars
批准号:
341270-2007
负责人:
Cami, Jan
金额:
$1.29万
依托单位国家:
加拿大
项目类别:
Discovery Grants Program - Individual
财政年份:
2008
资助国家:
加拿大
项目状态:
已结题
起止时间:
2008-01-01 至 2009-12-31
中文摘要
很多人都听过这句流行语:“我们是由星尘组成的”。事实上,在一个真正的宇宙生命周期中,恒星、行星和它们的居民是从早已逝去的恒星的灰烬中诞生的,但我们自己的化学成分证明了它们的存在。事实上,我们现在知道,所有的元素,如碳和氧,都是在恒星内部产生的。然而,这种星尘究竟是如何形成的,以及它的确切化学成分是什么,还不是很清楚。
英文摘要
Many people have heard the popular catchphrase "We are made of stardust". Indeed, in a truly cosmic lifecycle, stars, planets and their inhabitants are born from the ashes of stars that have long gone, but whose existence is evidenced by our very own chemical composition. Indeed, we now know that all elements like carbon and oxygen are produced in the interior of stars. Exactly how this stardust is formed however, and what its exact chemical composition is, is not well known.
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批准号:341270-2007
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项目类别:Discovery Grants Program - Individual
-
资助金额:$1.29万
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财政年份:2009
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负责人:Cami, Jan
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依托单位:
Molecules and dust around AGB stars
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批准号:341270-2007
-
项目类别:Discovery Grants Program - Individual
-
资助金额:$1.29万
-
财政年份:2007
-
负责人:Cami, Jan
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依托单位:
海外基金