ARG0000hhc elongated, bent, warped, triple, hosts?
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by
ChrisMolloy
Here's ARG0000hhc, which appears to be an #elongated, #warped, #bent #triple, with a background #compact emission.
The contour overlay image in this post was created from sources, and using methods, described in this RGZ Talk
thread.The host for the #triple emission appears to be SDSS J074927.24+520232.5, which has a z_sp=0.068 +/- 0.00001. This galaxy has a number of radio references in NED and SIMBAD, and has an ALLWISE reference, ALLWISE J074927.24+520232.6. NED and Simbad also list the environment of this galaxy as being part of a #cluster, which possibly explains the #bent, #warped, #elongated, morphology of the main emission.
To the south of the apparent #triple is a #compact emission, with the galaxy host possibly being SDSS J074925.25+520141.8, which has a z_ph=0.875 ± 0.0783. This object is slightly E of the lobe, and has an ALLWISE reference, ALLWISE J074925.16+520141.9.
Finally, this emission is cross referenced in the How to describe the radio morphology? thread, and the question has been raised whether there is also a further host for the central #triple emission. There is an AlLWISE emission, ALLWISE J074924.94+520213.1 for SDSS J074924.89+520213.3, which has a z_ph=0.105 ± 0.0134.
Also, there is a radio reference in NED for SDSS J074924.22+520222.2, which has a z_ph=0.305 ± 0.0716.
So, there is the possibility of other radio hosts being the cause of this emission, as well as it being in a #cluster.
As always, comments, suggestions, welcome.
Posted