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A&A 447, 63-70 (2006)
DOI: 10.1051/0004-6361:20053996
Hybrid morphology radio sources from the FIRST survey
M. P. Gawronski, A. Marecki, M. Kunert-Bajraszewska and A. J. KusTorun Centre for Astronomy, N. Copernicus University, 87-100 Torun, Poland
e-mail: amr@astro.uni.torun.pl
(Received 5 August 2005 / Accepted 13 September 2005 )
Abstract
The so-called HYbrid MOrphology Radio Sources (HYMORS) are a class of
objects that appear to have a mixed Fanaroff-Riley (FR) morphology in a single
object; i.e. a HYMORS has an FR I-type lobe on one side of its nucleus and
an FR II-type lobe on the other side. Because of this unique feature and given
that the origin of the FR morphological dichotomy is still unclear, HYMORS may
possibly play a crucial role in our understanding of the FR-dichotomy. As the
number of known HYMORS is quite small, we aimed to increase that number by
inspecting a few areas of the sky covered by the VLA FIRST survey and by
selecting 21 HYMORS candidates based on the morphology shown in the FIRST
images. They were observed with the VLA in B-conf. at
4.9 GHz. Three objects from the initial sample turned out to be actual
HYMORS and two others very likely to fulfill the criteria. These five were
subsequently re-observed with the VLA in A-conf. at 1.4 GHz. Our results
provide strong support to the findings of Gopal-Krishna & Wiita (2000, A&A, 363, 507), namely that there
are two different kinds of jets in HYMORS; consequently, the existence of
FR-dichotomy as a whole is difficult to reconcile with the class of
explanations that posit fundamental differences in the central engine.
Key words: radio continuum: galaxies -- galaxies: active -- galaxies: jets -- galaxies: nuclei
SIMBAD Objects
© ESO 2006
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