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銀河系の大局的 [C II] 158μm 放射
https://jaxa.repo.nii.ac.jp/records/33059
https://jaxa.repo.nii.ac.jp/records/33059a2f832f8-a488-4cc4-8837-49c5f83b4213
名前 / ファイル | ライセンス | アクション |
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SA0166913.pdf (898.4 kB)
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Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
タイトル | 銀河系の大局的 [C II] 158μm 放射 | |||||
言語 | ||||||
言語 | jpn | |||||
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 | departmental bulletin paper | |||||
その他のタイトル(英) | ||||||
その他のタイトル | LARGE-SCALE [CII] 158μm EMISSION OF THE GALAXY | |||||
著者 |
芝井, 広
× 芝井, 広× 奥田, 浩之× 中川, 貴雄× 松原, 英雄× 舞原, 俊憲× 水谷, 耕平× 小林, 行泰× 広本, 宣久× 西村, 徹郎× SHIBAI, Hiroshi× OKUDA, Haruyuki× NAKAGAWA, Takao× MATSUHARA, Hideo× MAIHARA, Toshinori× MIZUTANI, Kohei× KOBAYASHI, Yukiyasu× HIROMOTO, Norihisa× LOW, Frank J.× NISHIMURA, Tetsuo |
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著者所属 | ||||||
京都大学理学部 | ||||||
著者所属 | ||||||
京都大学理学部 | ||||||
著者所属 | ||||||
東京大学天文教育センター | ||||||
著者所属 | ||||||
郵政省通信総合研究所 | ||||||
著者所属 | ||||||
アリゾナ大学スチュワード天文台 | ||||||
著者所属 | ||||||
アリゾナ大学スチュワード天文台 | ||||||
出版者 | ||||||
出版者 | 宇宙科学研究所 | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science | |||||
書誌情報 |
宇宙科学研究所報告. 特集: 大気球研究報告 巻 24, p. 149-162, 発行日 1989-12 |
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抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | 銀河面に沿った広い領域から, 広がった[CII]157.74μm放射を検出した。観測は気球搭載赤外線望遠鏡に液体ヘリウム冷却のファブリ・ペロー分光器を搭載して行われた。強い[CII]放射が銀経30°から51°のほぼ全ての領域で検出された。この放射のほとんどは個別のHII領域に付随していない拡散成分である。[CII]放射の銀緯分布, 銀経分布は100μm連続波, および^<12>CO(1-0)に良く似ている。この[CII]放射は, 分子雲の表面に形成された「広がった光解離領域」から放射されている可能性が高い。銀河系の全[CII]光度は約3×10^7L_⦿で, 全遠赤外光度の約0.35%にあたる。 | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Diffuse [C II] line emission at 157.74μm has been observed in an extensive region along the Galactic plane, using a ballon-borne infrared telescope incorporated with a liquid helium cooled Fabry-Perot spectrometer. Strong emission has been ubiquitously detected all over the region between 1=30°and 51°. Most of the emission seems to be diffuse and unassociated with discrete HII regions. The longitude profile of the integrated [C II] intensity distribution is similar to those of IRAS 100μm and ^<12>CO (1-0) but not to that of HI 21cm. The large-scale diffuse [C II] emission probably comes from surfaces of molecular clouds which from diffuse photodissociation regions. The total [C II] luminosity of the Galaxy amounts to 2.6×10^7 L_⦿ which corresponds to about 0.35% of the total far-infrared luminosity. | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0285-9920 | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AN00354485 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: SA0166913000 |