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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4408

Title: Binary system of tailed radio galaxies
Authors: Klamer, I.
Subrahmanyan, Ravi
Hunstead, R.W.
Keywords: galaxies
interactions
galaxies: jets
large-scale structure of Universe
radio continuum: galaxies
Issue Date: Jun-2004
Publisher: Blackwell Publishing for the Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 2004, Vol.351, p101-109.
Abstract: We present a detailed study of a binary system of tailed radio galaxies which, along with 3C 75, is the only such binary known to exist. The binary is located in a region of low galaxy density at the periphery of a poor cluster Abell S345, but lies close to the massive Horologium-Reticulum supercluster. The radio sources have bent-tail morphologies and show considerable meandering and wiggling along the jets, which are collimated throughout their lengths. This work presents observations of the large-scale-structure environment of the binary tailed radio sources with a view to examining the influence of large-scale flows on the morphology and dynamics of the associated radio tails. We argue that the orbital motions of the host galaxies together with tidal accelerations toward the supercluster have resulted in the complex structure seen in these radio tails.
Description: Restricted Access.
URI: http://hdl.handle.net/2289/4408
ISSN: 0035-8711
1365-2966 (Online)
Alternative Location: http://adsabs.harvard.edu/abs/2004MNRAS.351..101K
http://arxiv.org/abs/astro-ph/0402574
http://dx.doi.org/10.1111/j.1365-2966.2004.07757.x
Copyright: 2004 Royal Astronomical Society
Appears in Collections:Research Papers (A&A)

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