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ISOCAM CVF OBSERVATIONS OF THE QUINTUPLET AND OBJECT17 CLUSTERS NEAR THE GALACTIC CENTER

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 – 3.08μm and 3.99 – 9.09μm. Emission of [Ar II] 6.99μm is detected in the “pistol-shaped” H II region (G0.150.05) to the south of theQuintuplet cluster. Absorption probably due to O-H stretching vibration (2.8μm) is evident in the Quintuplet spectra. In addition, Quintuplet members and the central part of Object #17 have CO2(4.3μm) and CO (4.7μm) absorption. Abundant CO2 might be present in these lines of sight.