FIRST "Winged" and X-Shaped Radio Source Candidates
Author(s) -
C. C. Cheung
Publication year - 2007
Publication title -
the astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.61
H-Index - 271
eISSN - 1538-3881
pISSN - 0004-6256
DOI - 10.1086/513095
Subject(s) - active galactic nucleus , physics , astrophysics , radio galaxy , surface brightness , supermassive black hole , astronomy , sample (material) , brightness , plasma , galaxy , quantum mechanics , thermodynamics
A small number of double-lobed radio galaxies (17 from our own census of theliterature) show an additional pair of low surface brightness `wings', thusforming an overall `X'-shaped appearance. The origin of the wings in theseradio sources is unclear. They may be the result of back-flowing plasma fromthe currently active radio lobes into an asymmetric medium surrounding theactive nucleus, which would make these ideal systems in which to studythermal/non-thermal plasma interactions in extragalactic radio sources. Anotherpossibility is that the wings are the aging radio lobes left over after a(rapid) realignment of the central supermassive black-hole/accretion disksystem due perhaps to a merger. Generally, these models are not well tested;with the small number of known examples, previous works focused on detailedcase studies of selected sources with little attempt at a systematic study of alarge sample. Using the VLA-FIRST survey database, we are compiling a largesample of winged and X-shaped radio sources for such studies. As a first steptoward this goal, an initial sample of 100 new candidate objects of this typeare presented in this paper. ...[abridged]
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