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Analysis of carbonaceous materials which show "217.5<plus-minus>2.5 nm hum

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”
批准号:
05640305
负责人:
SAKATA Akira
金额:
$1.34万
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
项目状态:
已结题
起止时间:
1993 至 1994

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中文摘要
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英文摘要
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.
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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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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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通讯作者:
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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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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通讯作者:
Emission Mechanism of Carbonaceous Interstellar and Circumstellar Dusts
  • 批准号:
    01540217
  • 项目类别:
    Grant-in-Aid for General Scientific Research (C)
  • 资助金额:
    $0.83万
  • 财政年份:
    1989
  • 负责人:
    SAKATA Akira
  • 依托单位:
海外基金