Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2878
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dc.contributor.authorSubrahmanyan, R-
dc.contributor.authorSaripalli, L-
dc.contributor.authorHunstead, R. W-
dc.date.accessioned2008-07-25T05:45:10Z-
dc.date.available2008-07-25T05:45:10Z-
dc.date.issued1996-03-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 279, No. 1, pp. 257 - 274en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/2878-
dc.description.abstractWe present radio images with the Australia Telescope of a sample of powerful radio galaxies. The observations were designed to be sensitive to the largest-scale structures in the radio sources. The morphologies are representative of radio galaxies with FRII type structures and with sizes exceeding 1Mpc. We observe the giant source to have the same axial ratios as those in smaller sources with similar radio powers. Moreover, the deviations from axial symmetry are also observed to be linearly scaled from sources an order of magnitude smaller. The observations are indicative of self-similar evolution in the morphologies of powerful radio galaxies.en
dc.format.extent3299049 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherRoyal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996MNRAS.279..257Sen
dc.subjectGalaxies:activeen
dc.subjectIntergalactic mediumen
dc.subjectRadio continuum: galaxiesen
dc.titleMorphologies in megaparsec-size powerful radio galaxiesen
dc.typeArticleen
Appears in Collections:IIAP Publications

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