Infrared images and photometry of the cluster near G 0.15 - 0.05

Details Infrared images and photometry of the cluster near G 0.15 - 0.05 Infrared images and photometry of the cluster near G 0.15 - 0.05

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.242p..55g&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 242, Feb. 1, 1990, p. 55P-58P.

Astronomy and Astrophysics

Astronomy

44

Infrared Photometry, Milky Way Galaxy, Star Clusters, Star Formation, Interstellar Extinction, Molecular Clouds, Polarized Radiation, Protostars, Stellar Spectra

Scientific paper

An unusual infrared cluster, first identified as a triplet of bright sources and later as a quintuplet, has been found near galactic coordinates l = 0.15 deg, b = 0.05 deg on images obtained with the ESO infrared array camera. The JHKL (1.2 to 3.4 microns) colors of several of the individual sources within the cluster are unusually red, leading them to be associated with a number of similar objects which are identified with luminous IRAS point sources near the Galactic Centre. It is suggested that they are recently formed early-type stars embedded in dust shells.

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