carbon star中文是什么意思

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中文翻译
造句

【天文学】碳星。

carbon n. 1.【化学】碳。 2.【电学】碳精棒[片、粉]；碳 ...
star n. 1.星；【天文学】恒星 (opp. planet) ...
carbon stars c star 碳星
dwarf carbon star 碳矮星
star-shaped carbon cell 星状碳极电池
star n. 1.星；【天文学】恒星 (opp. planet)。 2.星状物，星(形勋)章。 3.【印刷】星形号〔*〕。 4.【占星术】〔常pl.〕命星；〔pl.〕命运，运气。 5.名演员，明星；〔口语〕著名人物。 6.【林业】?。 7.【动物；动物学】海星。 8.(马额等的)白斑。 a falling [shooting] star流星。 a fixed star恒星。 this star 〔诗〕地球。 His star was in the ascendant. 他(那时)正在走运。 My stars! ＝〔戏谑语〕 My stars and garters! 哎呀!天哪!〔表示吃惊〕。 The stars were against it. 那注定要失败的。 the S- Chamber 【英史】星室法庭〔以暴虐专横著称〕。 be born under a lucky [an unlucky] star 生在幸福[不幸]中。 curse one's stars 怨恨自己不走运。 march by the stars 【军事】看星行进。 see stars 〔口语〕眼里冒金星。 all star cast 【戏剧】全部角色由名演员扮演。 thank one's stars 觉得运气好，觉得幸福。 trust to one's star相信自己的运气。 vt. (starred starring) 1.用星(形物)装饰；加星号。 2.使…成为明星，使演主角。 vi. 1.星一般地辉耀。 2.作出杰出成就。 3.(演员)主演 (in); 成为明星[名演员]。 4.(打台球或玩 domino 输掉而失权的人)出钱购买继续游戏的权利。 They starred her for the first time. 他们第一次以她为主角。 She has starred in many pictures. 她已主演多部影片。
star the 明星报; 星报
the star 巨星本色; 星星之章; 昨日星尘
carbon n. 1.【化学】碳。 2.【电学】碳精棒[片、粉]；碳精电极。 3.(一张)复写纸。 4.复写的副本。 a carbon of a letter 一封信的副本。
mill star，jack star，star 星形铁(滚光用)
film star movie star 电影餍
film star，movie star 电影明星
jackstar，mill star，star 星形铁(滚光用)
silver star and golden star 金星和银星
star doublet(star tripet) 星彩垫层宝石
star finder = star identifier 索星卡
star identifier = star finder 索星卡
star light，star bright 星星闪，星星亮
star singer; singing star 歌星
star star connection 星-星接法; 星形星形结线
star,fixed star 恒星
star-dot-star 星点星文件名
star-star connection 星星形接线; 星形-星形连接; 星形星形结线
star，jackstar，mill star 星形铁(滚光用)
breakaway of carbon-carbon bond 碳-碳键断裂

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例句与用法

Usually , carbon stars can be divided into three groups : visual carbon stars , infrared carbon stars and extreme carbon stars
通常，碳星又主要分为光学碳星、红外碳星以及极端碳星。
Carbon stars with c / o > 1 are a kind of stars that form at the agb stage and evolved from oxygen - rich agb stars with mid - mass
碳星是中等质量星演化到agb阶段时可能形成的一种恒星，它由氧星演化而来， [ c o ] 1 。
These stars are undergoing important mass loss process and are likely to represent a more evolved phase of the stellar evolution than visual carbon stars
红外碳星经历了重要的质量损失过程，是光学碳星演化的后期。
This present paper is contributed to the study of the evolutionary nature of iso sws spectra from carbon - rich agb stars ( carbon stars ) and molecular and dust features around such carbon stars
本文主要致力于研究富碳agb星的isosws红外光谱的演化和它的分子、尘埃特征。
After competing our work , some conclusions expected are obtained for the evolutionary principles of carbon stars and the evolutionary nature of molecule and dust features around them
在对它们的研究和分析后得到了我们所期待的关于碳星的一些演化规律和分子、尘埃特征的演化特性。
By using the iso sws spectra we have studied their physical nature including their molecular and dust features in the circumstellar envelope to make us understand the evolutionary status of carbon stars
这29颗sic碳星的isosws光谱能很好地反映碳星的演化，有助于我们了解碳星的演化及其分子、尘埃特征。
The extreme carbon stars , whose derived mass loss rates and optical depths are both very high , are more evolved than infrared carbon stars . these stars are expected to evolve into protoplanatary nebula soon
极端碳星是高度演化后的红外碳星，它的质量损失率及光深都非常高，几乎没有其光学对应体，并将很快演化为前行星状星云。
The infrared carbon stars , whose infrared spectra are mainly due to the dust emission in the circumstellar envelope , are usually believed to be surrounded by the carbon rich envelope characterized by the sic emission feature at 11 . 3um
红外碳星常被认为有很厚的富碳拱星壳层，它的红外光谱主要表现为源于拱星壳层的尘埃发射，这个尘埃发射主要以11 . 3 m的sic发射为标记。
We have elected 29 carbon stars with sic emission feature at 11 . 3um , i . e . sic carbon stars , which include visual carbon stars , infrared carbon stars and extreme carbon stars to be our working samples in this paper
本文将选取29颗富碳agb星作为研究对象，它们均有11 . 3 msic发射特征，在本文中称之为碳化硅碳星( sic碳星) ，它们覆盖了光学碳星、红外碳星和极端碳星的阶段。
Visual carbon stars whose mid - infrared spectra are mainly dominated by photospheric continuum and show large excesses at 60um , represent a transition phase which follows an interruption of mass loss from the oxygen - rich phase and begins a new phase of the mass loss of carbon - rich material . excesses at 60um in these stars are the emission from the residual of oxygen - rich material
光学碳星的中红外能量主要来自光球，在60 m处存在超量发射，人们认为其演化阶段处在抛射富氧物质终止和新的富碳拱星壳层形成之间，其60 m超量发射就是富氧物质的残余效应。

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百科解释

A carbon star is a late type star similar to a red giant (or occasionally to a red dwarf) whose atmosphere contains more carbon than oxygen; the two elements combine in the upper layers of the star, forming carbon monoxide, which consumes all the oxygen in the atmosphere, leaving carbon atoms free to form other carbon compounds, giving the star a "sooty" atmosphere and a strikingly red appearance.

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