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Large-scale mapping observations of the CI 3P1-3P0 line toward heiles cloud2 in the Taurus Dark Cloud
http://hdl.handle.net/10098/1529
http://hdl.handle.net/10098/1529e87bfa91-c079-4ecd-8e06-463275367a41
名前 / ファイル | ライセンス | アクション |
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Astrophysical_Journal__________________________524,_L129-L132.pdf (1.1 MB)
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〓 1999 American Astronomical Society
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Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2008-02-01 | |||||
タイトル | ||||||
タイトル | Large-scale mapping observations of the CI 3P1-3P0 line toward heiles cloud2 in the Taurus Dark Cloud | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | ISM | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | atoms—ISM | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | clouds—ISM | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | evolution—ISM | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | individual (Heiles's cloud 2) | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_1843 | |||||
資源タイプ | other | |||||
著者 |
MAEZAWA, Hiroyuki
× MAEZAWA, Hiroyuki× IKEDA, Masafumi× ITO, Tetsuya× SAITO, Gaku× SEKIMOTO, Yutaro× YAMAMOTO, Satoshi× TATEMATSU, Ken-ichi× ARIKAWA, Yuji× ASO, Yoshiyuki× NOGUCHI, Takashi× SHI, Sheng-Cai× MIYAZAWA, Keisuke× SAITO, Shuji× OZEKI, Hiroyuki× FUJIWARA, Hideo× OHISHI, Masatoshi× INATANI, Junji |
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抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | A distribution of the neutral carbon atom (C i) in Heiles cloud 2 (HCL2) has been investigated with the Mount Fuji submillimeter-wave telescope. A region of 1.2 deg2 covering a whole region of HCL2 has been mapped with the 3P1?3P0 fine-structure line (492 GHz) of C i. The global extent of the C i emission is similar to that of 13CO, extending from southeast to northwest. However, the C i intensity is found to be rather weak in dense cores traced by the line of C18O. On the other hand, strong C i emission is observed in a south part of HCL2 in which the C18O intensity is fairly weak. The C i/CO abundance ratio is greater than 0.8 for the C i peak, whereas it is 0.1 for the dense cores such as the cyanopolyyne peak. The C i?rich cloud found in the south part may be in the early evolutionary stage of dense core formation where C i has not yet been converted completely into CO. This result implies that formation of dense cores is taking place from north to south in HCL2. | |||||
書誌情報 |
The Astrophysical Journal 巻 524, p. L129-L132, 発行日 1999-10 |
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出版者 | ||||||
出版者 | University of Chicago Press | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0004637X | |||||
書誌レコードID | ||||||
識別子タイプ | NCID | |||||
関連識別子 | TD00007820 | |||||
DOI | ||||||
関連タイプ | isVersionOf | |||||
識別子タイプ | DOI | |||||
関連識別子 | 10.1086/312316 | |||||
著者版フラグ | ||||||
出版タイプ | AO | |||||
出版タイプResource | http://purl.org/coar/version/c_b1a7d7d4d402bcce |