File:3c83p1 21cm opt 6in hi.tif

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Description

Radio Galaxy 3C83.1B

About this Image

This is a false-color image of the wide-angle radio galaxy 3C83.1B, associated with the elliptical galaxy NGC1265 in the Perseus Cluster of galaxies. Blue colors show the distribution of stars, made from an image from the Digitized Second Palomar Sky Survey, and red colors show the radio radiation as imaged by the VLA, measured at a wavelength of 20cm. The galaxy is moving through the intergalactic medium of the Perseus Cluster at a velocity of about 2000 km/s. It is thought that twin beams of plasma ejected from the galactic nucleus are bent by the ram pressure exerted by the external gas, producing the 'U' shape. The radio tail extends much further than is visible in this image (see icon for 3C 83.1B at The DRAGN's Atlas page).

Investigator(s): C. P. O'Dea & F. N. Owen. Optical/Radio superposition by Alan Bridle


Technical Data


   Telescope 	VLA 
   Date of Observation 	1981-11-12 
   Type of Observation 	Continuum Observations 
   Band 	L 
   Wavelength 	20 cm 
   Frequency 	1.4 GHz 
   Center of Image 	RA: 03:18:15.80, Dec: 41:51:28.00 (J2000)  
   Field of View 	0.2167 x 0.2333 degrees  
   Technical Caption 	Radio data: VLA C+D array L-band (20cm) observation, 12" resolution.  
.
Date (of Observation) 1981-11-12
Source

http://images.nrao.edu/images/3c83p1_21cm_opt_6in_hi.tif

http://images.nrao.edu/AGN/Radio_Galaxies/333
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Date/TimeThumbnailDimensionsUserComment
current22:05, 26 September 2017Thumbnail for version as of 22:05, 26 September 20172,712 × 3,600 (11.34 MB)Fabian RRRR (talk | contribs)== {{int:filedesc}} == {{Information |Description=Radio Galaxy 3C83.1B About this Image This is a false-color image of the wide-angle radio galaxy 3C83.1B, associated with the elliptical galaxy NGC1265 in the Perseus Cluster of galaxies. Blue colors...

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