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Large-Scale Mapping Observations of the C i (3P1–3P0) and CO (J = 3–2) Lines toward the Orion A Molecular Cloud
http://hdl.handle.net/10098/1532
http://hdl.handle.net/10098/1532d7c724fa-fff8-4171-aae4-a4ed049dcd4b
名前 / ファイル | ライセンス | アクション |
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BD00007832_001.pdf (785.0 kB)
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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 | 2008-02-04 | |||||
タイトル | ||||||
タイトル | Large-Scale Mapping Observations of the C i (3P1–3P0) and CO (J = 3–2) Lines toward the Orion A Molecular 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 | individual (Orion A Cloud)—ISM | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | molecules | |||||
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 |
IKEDA, Masafumi
× IKEDA, Masafumi× MAEZAWA, Hiroyuki× 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 | Large-scale mapping observations of the 3P1–3P0 fine-structure transition of atomic carbon (C i, 492 GHz) and the transition of CO (346 GHz) toward the Orion A molecular cloud have been carried out with the Mount Fuji submillimeter-wave telescope. The observations cover 9 deg2 and include the Orion Nebula M42 and the L1641 dark cloud complex. The C i emission extends over almost the entire region of the Orion A cloud and is surprisingly similar to that of 13CO (). The CO () emission shows a more featureless and extended distribution than C i. The C i/CO () integrated intensity ratio shows a spatial gradient running from the north (0.10) to the south (1.2) of the Orion A cloud, which we interpret as a consequence of the temperature gradient. On the other hand, the C i/13CO () intensity ratio shows no systematic gradient. We have found a good correlation between the C i and 13CO () intensities over the Orion A cloud. This result is discussed on the basis of photodissociation region models. | |||||
書誌情報 |
Astrophysical Journal 巻 527, p. L59-L62, 発行日 1999-12 |
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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 | TD00007832 | |||||
DOI | ||||||
関連タイプ | isVersionOf | |||||
識別子タイプ | DOI | |||||
関連識別子 | 10.1086/312395 | |||||
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 |