We looked for the optical counterparts for every of the newly discovered XRGs and ZRGs using the Sloan Digital Sky Survey (SDSS) data catalogue (Gunn et al., 2006; Alam et al., 2015). The identification of the optical/IR counterpart of the winged radio galaxy was based on the position of the optical/IR source relative to the radio galaxy morphology. In columns 3 and 4 of Table 1 and Table 2, the positions of newly identified XRGs and ZRGs are talked about where the place of optical host galaxies are used when obtainable. As is the case for the inverted files used to carry out fielded searches on the contents of the bibliographic entries in our database (see part 3), each property table is decomposed in two components, an index file and an inventory file. On this part, we additionally outline how we separate the XRGs and ZRGs from the whole winged candidate record. Proctor (2011) introduced a list of 156 XRG candidates by automated morphology detection course of. The discussion and conclusion are offered in part 5 and part 6 respectively. Part 3 contains the results of our search that includes the properties of XRGs and ZRGs. Relying on the position of the wings, the winged radio galaxies might be categorized into two distinct teams – X-shaped radio galaxies (XRGs) and Z-shaped radio galaxies (ZRGs).

3C 272.1 is the first recognized winged supply that has Z-shaped morphology (Riley, 1972). Ekers et al. The morphology of sources is determined by the radio contour levels (particularly the lowest contour) and the sign to noise. 0.5), which is typical of lobe dominated radio galaxies. In some cases, it originated from near the central core of the galaxy and aligns with the primary jets, gives rise to an X-formed construction and named as X-shaped radio galaxies (XRGs). Out of a total of 21 sources, optical/IR counterparts are discovered for 14 sources for XRGs (sixty six per cent). A complete of 33 winged sources are discovered, out of which 21 are XRGs, and the remaining 12 are ZRGs. Utilizing The TIFR GMRT Sky Survey (TGSS) at one hundred fifty MHz, Bhukta, Pal & Mondal (2020) detected 92 winged sources out of which 68 are XRGs and 24 are ZRGs. Instance of six XRGs and ZRGs are introduced in Determine 1 and Determine 2, respectively. The essential parameters of newly recognized XRGs and ZRGs are talked about in Desk 1 and Table 2 respectively. Optical counterparts are recognized for 14 XRGs (67 per cent) and 12 ZRGs (a hundred per cent).

The statistical research are executed on the relative dimension of the foremost and minor axes and the angle between the main axis and minor axis for XRGs. This change within the spin axis could also be the reason for producing the secondary lobes for the radio galaxy (Gopal-Krishna, Biermann & Witta, 2003; Zier, 2005). (iii) Precession of jets (Rottmann, 2001; Dennett-Thorpe et al., 2002): According to this model, it is believed that the secondary lobes are the remnants which are leftover from a speedy realignment of the central supermassive black gap-accretion disk system (Dennett-Thorpe et al., 2002). it can be stated that the wings are due to the relic emission of the beforehand lively lobes (Rottmann, 2001) whose path of emission has been modified with time. When the secondary lobes appear to return out from the central core or close to the central region, we categorize those sources as X-formed sources. We pointed out some broadly mentioned models- (i) Backflow of plasma (Leahy & Williams, 1984; Capetti et al., 2001): This model means that the formation of wings in winged radio galaxies are as a result of backflow of plasma from the central hotspot and this backflow happens when jet materials is speculated to be released by the hotspots and then streaming again in direction of the host galaxy.

Climates with long and chilly winters that get a lot of sunshine could get the most out of a photo voltaic air heater. Twisted nematics get their name as a result of they’re twisted in their natural state. The actual French fry is an American invention but obtained its title based on the origin nation of fried potatoes. The origin of the formation of wings (secondary jets) could be very mysterious and is required a really deep study. Jy for all photographs to make a uniform research. SDSS photos are overlaid with LOTSS DR1 photos. With the help of the Very Massive Array (VLA), Faint Photos of Radio Sources at Twenty cm (FIRST) survey at 1.Four GHz, Cheung (2007) introduced a pattern of one hundred winged sources. Twin AGN (Lal & Rao, 2005, 2007): In response to this model the formation of wings is due to two pairs of jets are believed to be ejected from two unresolved AGNs in a special path.