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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4390

Title: SGRS J0515-8100: a fat-double giant radio galaxy
Authors: Subrahmanyan, Ravi
Hunstead, R.W.
Cox, N.L.J.
McIntyre, V.
Keywords: individual (SGRS J0515-8100)
Galaxies
Interactions
Jets
Nuclei
Intergalactic Medium
Radio Continuum
Issue Date: Jan-2006
Publisher: The University of Chicago Press for the American Astronomical Society
Citation: Astrophysical Journal, 2006, Vol.636, p172-180
Abstract: We present here the first detailed study of a giant radio galaxy of the fat-double type. The lobes of the double radio galaxy SGRS J0515-8100 have transverse widths that are 1.3 times their extent from the center, their surface brightness is the lowest among known giant radio sources, and the lobes have relatively steep radio spectra. We infer that these wide lobes were created as a result of a highly variable and intermittent jet whose axis direction also varied significantly: the fat-double lobes in this giant radio source are a result of the ejection and deposition of synchrotron plasma over a wide range of angles over time rather than the expansion of relic lobes. In addition, the optical host shows evidence for an ongoing galaxy-galaxy interaction. SGRS J0515-8100 supports the hypothesis that interactions with companions might perturb the inner accretion disk that produces and sustains the jets at the centers of active galactic nuclei. As a result, it appears unnecessary to invoke black hole coalescence to explain such morphologies, implying that the corresponding event rates predicted for gravitational wave detectors may be overestimates.
Description: Restricted Access.
URI: http://hdl.handle.net/2289/4390
ISSN: 0004-637X
1538-4357 (Online)
Alternative Location: http://adsabs.harvard.edu/abs/2006ApJ...636..172S
http://arxiv.org/abs/astro-ph/0509275
http://dx.doi.org/ 10.1086/497956
Copyright: 2006 American Astronomical Society
Appears in Collections:Research Papers (A&A)

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