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Identification of New Near-Infrared Diffuse Interstellar Bands in the Orion Nebula
http://hdl.handle.net/10091/10125
http://hdl.handle.net/10091/101254644fbf0-a51e-4940-91af-be301968d8c4
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
ApJ_700_1988.pdf (431.7 kB)
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| Item type | 学術雑誌論文 / Journal Article(1) | |||||
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| 公開日 | 2010-06-04 | |||||
| タイトル | ||||||
| タイトル | Identification of New Near-Infrared Diffuse Interstellar Bands in the Orion Nebula | |||||
| 言語 | ||||||
| 言語 | eng | |||||
| DOI | ||||||
| 関連識別子 | https://doi.org/10.1088/0004-637X/700/2/1988 | |||||
| 関連名称 | 10.1088/0004-637X/700/2/1988 | |||||
| キーワード | ||||||
| 主題 | ISM: individual (Orion Nebula), ISM: lines and bands, ISM: molecules | |||||
| 資源タイプ | ||||||
| 資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
| 資源タイプ | journal article | |||||
| 著者 |
Misawa, T
× Misawa, T× Gandhi, P× Hida, A× Tamagawa, T× Yamaguchi, T |
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| 信州大学研究者総覧へのリンク | ||||||
| 表示名 | Misawa, T | |||||
| URL | http://soar-rd.shinshu-u.ac.jp/profile/ja.ypchuUkV.html | |||||
| 出版者 | ||||||
| 出版者 | The American Astronomical Society | |||||
| 引用 | ||||||
| 内容記述タイプ | Other | |||||
| 内容記述 | The Astrophysical Journal. 700:1988-1993 (2009) | |||||
| 書誌情報 |
The Astrophysical Journal 巻 700, 号 2, p. 1988-1993, 発行日 2009-08-01 |
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| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | Large organic molecules and carbon clusters are basic building blocks of life, but their existence in the universe has not been confirmed beyond doubt. A number of unidentified absorption features (arising in the diffuse interstellar medium), usually called "Diffuse Interstellar Bands" (DIBs), are hypothesized to be produced by large molecules. Among these, buckminsterfullerene C60 has gained much attention as a candidate for DIB absorbers because of its high stability in space. Two DIBs at lambda similar to 9577 angstrom and 9632 angstrom have been reported as possible features of C-60(+). However, it is still not clear how their existence depends on their environment. We obtained high-resolution spectra of three stars in/around the Orion Nebula, to search for any correlations of the DIB strength with carrier's physical conditions, such as dust abundance and UV radiation field. We find three DIBs at lambda similar to 9017 angstrom, 9210 angstrom, and 9258 angstrom as additional C-60(+) feature candidates, which could support this identification. These DIBs have asymmetric profiles similar to the longer wavelength features. However, we also find that the relative strengths of DIBs are close to unity and differ from laboratory measurements, a similar trend as noticed for the 9577/9632 DIBs. | |||||
| 資源タイプ（コンテンツの種類） | ||||||
| 内容記述タイプ | Other | |||||
| 内容記述 | Article | |||||
| ISSN | ||||||
| 収録物識別子タイプ | ISSN | |||||
| 収録物識別子 | 0004-637X | |||||
| 書誌レコードID | ||||||
| 収録物識別子タイプ | NCID | |||||
| 収録物識別子 | AA00553253 | |||||
| 出版タイプ | ||||||
| 出版タイプ | VoR | |||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
| WoS | ||||||
| 表示名 | Web of Science | |||||
| URL | http://gateway.isiknowledge.com/gateway/Gateway.cgi?&GWVersion=2&SrcAuth=ShinshuUniv&SrcApp=ShinshuUniv&DestLinkType=FullRecord&DestApp=WOS&KeyUT=000268098100084 | |||||
