SIMBAD references

1996A&A...315L.205N - Astronomy and Astrophysics, volume 315, L205-208 (1996/11-2)

ISOCAM CVF observations of the Quintuplet and Object#17 clusters near the Galactic Center.

NAGATA T., KAWARA K., ONAKA T., KITAMURA Y. and OKUDA H.

Abstract (from CDS):

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 (G0.15-0.05) to the south of the Quintuplet 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.

Abstract Copyright: ∼

Journal keyword(s): dust, extinction - H II regions - ISM: molecules - Galaxy: center - infrared: interstellar: lines

CDS comments: Object 17 = [NHS93] 17

Simbad objects: 17

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