Region of recent star formation in our Galaxy: continuum emission at 2 cm
from the thermal radio source DR 21
observed at a resolution of 2 arcsec. The intesnsity is color-coded from blue (> 50 to 200 mJy/beam) to red (> 400 to a maximum of 600 mJy/beam). DR 21 is comprised of four ultracompact HII regions, each of which is excited by a recently-formed hot O or B star. The most intense HII region C (bottom) is about 10 arcsec across or 0.3 light-years (at a distance of 6000 light-years).
Investigator(s): H.R. Dickel, A.F. Lubenow, W.M. Goss, and A.H. Rots
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Telescope
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VLA
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Date of Observation
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1983-05-16
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Type of Observation
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Continuum Observations
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Band
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U
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Wavelength
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2.0 cm
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Frequency
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15 GHz
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Center of Image
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RA: 20:37:14.30, Dec: 42:09:3.00 (B1950)
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Field of View
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0.0167 x 0.0167 degrees
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Technical Caption
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Observing run - 1983 May 14 & 16 at the VLA in the C-configuration using 17
antennas.
Type of observation - spectral line mapping.
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- Astronomical database entries for DR21
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