A new near-infrared source in the molecular cloud associated with S106

Details A new near-infrared source in the molecular cloud associated with S106 A new near-infrared source in the molecular cloud associated with S106

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...116..179h&link_type=abstract

Astronomy and Astrophysics, vol. 116, no. 1, Dec. 1982, p. 179-182.

Astronomy and Astrophysics

Astrophysics

1

Hydrogen Clouds, Infrared Spectra, Molecular Clouds, Near Infrared Radiation, Nebulae, Point Sources, Astronomical Maps, Calibrating, Carbon Monoxide, Continuous Spectra

Scientific paper

A near-infrared pointlike source was detected in the central part of the S106 molecular cloud, and a medium-resolution (8 kaysers) spectrum was measured between 1.25 and 2.50 microns. The spectrum consists of a flat portion at wavelengths below 1.82 microns and a steep part in the range above 2.04 microns. The maximum flux is 0.9 Jy at 2.22 microns. The v equals 2-0 absorption band is detected, and the upper limit on the integrated B-gamma flux is 2 x 10 to the -16th W/sq m.

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