Analysis of carbonaceous materials which show "217.5<plus-minus>2.5 nm hum
碳质材料分析显示“217.5<正负>2.5 nm 嗡嗡声”
基本信息
- 批准号:05640305
- 负责人:
- 金额:$ 1.34万
- 依托单位:
- 依托单位国家:日本
- 项目类别:Grant-in-Aid for General Scientific Research (C)
- 财政年份:1993
- 资助国家:日本
- 起止时间:1993 至 1994
- 项目状态:已结题
- 来源:
- 关键词:
项目摘要
Interstellar extinction curve is a spectrum of interstellar dust in our Galaxy. In the spectrum we can see a clear 217.5 nm hump and and very broad-500 nm hump.QCC (Quenched Carbonaceous Composite) is an amorphous carbonaceous material formed from a hydrocarbon plasma. In a previous paper (Sakata et al.1994), we have studied two forms of QCC : a dark QCC component located near the plasmic beam and a thermally-altered filmy QCC.Both types of QCC derivatives show an absorption feature near 217 nm but with different extinction magnitude. And we showed that soots produced from methane, methane-hydrogen gas mixtures, have a broad extinction feature centered at about 217 nm.In this work we present a new material, mesophase pitch, which has a 217 nm extinction feature. The mesophase pitch was produced from raw pitch by heating to -450 C,by Asahi Coke Ltd. Chemical analysis of the mesophase pithc showed H/C=0.52.These three kinds of materials showing about 217 nm hump were formed under hydrogen rich environment. From the chemical composition of mesophase pitch, we can deduce that the carbonaceous materials having 217 nm feature contain a large amount of hydrogen in their structure.
星际消光曲线是我们银河系中星际尘埃的光谱。在光谱中,我们可以看到一个清晰的217.5 nm峰和一个非常宽的500 nm峰。QCC(淬火碳质复合材料)是一种由碳氢化合物等离子体形成的无定形碳质材料。在之前的一篇论文(Sakata et al.1994)中,我们研究了两种形式的QCC:位于等离子束附近的暗QCC组件和热改变的薄膜QCC。两种QCC衍生物在217 nm附近均有吸收,但消光幅度不同。我们发现,由甲烷,甲烷-氢气混合物产生的煤烟,在217纳米处有广泛的消光特征。在这项工作中,我们提出了一种新的材料,中间相沥青,具有217纳米消光特性。中间相沥青由原沥青加热至-450℃,由朝日焦炭有限公司生产。化学分析表明,H/C=0.52。这三种材料都是在富氢环境下形成的,峰长约217 nm。从中间相沥青的化学组成可以推断出217 nm特征的碳质材料结构中含有大量的氢。
项目成果
期刊论文数量(12)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
A.Sakata, S.Wada, A.T.Tokunaga, T.Narisawa, H.Nakagawa, and H.Ono: ""Ultraviolet Spectra of Quenched Carbonaceous Composite Derivatives : Comparison to the "217 nm" Interstellar Absorption Feature."" Astrophys.J.430, No.1. 311-316 (1994)
A.Sakata、S.Wada、A.T.Tokunaga、T.Narisawa、H.Nakakawa 和 H.Ono:“淬火碳质复合衍生物的紫外光谱:与“217 nm”星际吸收特征的比较。”Astrophys.J
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- 影响因子:0
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- 通讯作者:
A. Sakata, S. Wada, A. T. Tokunaga and T. Narisawa: "Comparison of the Absorption Curves of Soots, Pitch Samples, and QCCs to the Interstellar Extinction Curve." Planetary and Space Science,. (in press). (1995)
A. Sakata、S. Wada、A. T. Tokunaga 和 T. Narisawa:“烟灰、沥青样品和 QCC 的吸收曲线与星际消光曲线的比较”。
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- 影响因子:0
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Sakata,A.et.al.: "Ultraviolet Spectra of Quenched Carbonaceous Composite Derivative Comparison to the“217 Nanometer"Interstellar Absorption Feature" Astrophysical Journal. 430 in press. (1994)
Sakata, A.et.al.:“淬火碳质复合材料衍生物的紫外光谱与“217 纳米”星际吸收特征的比较”天体物理学杂志。430 版。(1994 年)
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- 影响因子:0
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- 通讯作者:
A. Sakata, S. Wada, A. T. Tokunaga, T. Narisawa, H. Nakagawa, and H. Ono: "Ultraviolet Spectra of Quenched Carbonaceous Composite Derivatives : Comparison to the“217nm"Interstellar Absorption Feature." Astrophys. J.,. 430. 311-316 (1994)
A. Sakata、S. Wada、A. T. Tokunaga、T. Narisawa、H. Nakakawa 和 H. Ono:“淬火碳质复合衍生物的紫外光谱:与“217nm”星际吸收特征的比较。”Astrophys. J.,. 430. 311-316 (1994)
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SAKATA Akira其他文献
SAKATA Akira的其他文献
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{{ truncateString('SAKATA Akira', 18)}}的其他基金
Emission Mechanism of Carbonaceous Interstellar and Circumstellar Dusts
碳质星际和星周尘埃的发射机制
- 批准号:
01540217 - 财政年份:1989
- 资助金额:
$ 1.34万 - 项目类别:
Grant-in-Aid for General Scientific Research (C)
相似海外基金
Study of Chemical Processing of Carbonaceous Dust
含碳粉尘化学处理研究
- 批准号:
14540224 - 财政年份:2002
- 资助金额:
$ 1.34万 - 项目类别:
Grant-in-Aid for Scientific Research (C)














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