Dance of the Radio Galaxies |
 | Minimum credit line: Image courtesy of NRAO/AUI
(for details, see .
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Four radio galaxies perform a complicated dance in the heart of Abell 2255, a rich cluster of galaxies in the throes of a cluster-cluster merger. The optical image, collected at Kitt Peak National Observatory, is displayed in blue and reveals numerous galaxies in a chain-like structure. The NRAO Very Large Array was used to obtain the radio data, which are shown in red. The prominent radio galaxies include three sources in which twin jets of radio-emitting plasma are swept back into a single tail by motion relative to the diffuse gas which permeates the cluster itself. Also visible are numerous fainter galaxies with associated radio emission. In many cases, these are starbursts likely instigated by the dramatic environment. Investigator(s): Neal Miller & Frazer Owen This image is available in the following downloadable versions:
- 400 x 533
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- 2027 x 2700
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Telescope
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VLA
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Date of Observation
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1998-07-00
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Type of Observation
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Continuum Observations
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Band
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L
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Wavelength
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20 cm
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Frequency
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1.4 GHz
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Center of Image
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RA: 17:12:30.30, Dec: 64:01:49.80 (J2000)
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Field of View
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0.2000 x 0.1500 degrees
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Technical Caption
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The optical image was obtained at KPNO using the 0.9m with the Mosaic CCD. The original pixel scale was 0.68" with seeing of about 1". The radio image is the result of numerous pointings combined in a mosaic. It corresponds to both B and D array VLA data, each at 1.4GHz. Exposure times per pointing were about 20 minutes (B array) and 10 minutes (D array), resulting in a net rms noise in the final mosaic map of under 40 uJy/beam.
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