1996年11月
ISOCAM CVF observations of the Quintuplet and Object#17 clusters near the Galactic Center
ASTRONOMY & ASTROPHYSICS
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- 巻
- 315
- 号
- 2
- 開始ページ
- L205
- 終了ページ
- L208
- 記述言語
- 英語
- 掲載種別
- 研究論文(学術雑誌)
- 出版者・発行元
- EDP SCIENCES S A
Two fields near the Galactic Center, containing the Quintuplet and Object #17 star-clusters, have been imaged with the ISOCAM circular variable filters (CVFs) in the wavelength range of 2.47 - 3.08 mu m and 3.99 - 9.09 mu m. Emission of [Ar II] 6.99 mu m is detected in the ''pistol-shaped'' H II region (G0.15-0.05) to the south bf the Quintuplet cluster. Absorption probably due to O-H stretching vibration (2.8 mu m) is evident in the Quintuplet spectra. In addition, Quintuplet members and the central part of Object #17 have CO2(4.3 mu m) and CO (4.7 mu m) absorption. Abundant CO2 might be present in these lines of sight.
- リンク情報
- ID情報
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- ISSN : 0004-6361
- Web of Science ID : WOS:A1996VU26600043