Good target for studying how the neighborhood affects jets and lobes?
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by JeanTate
The odd morphology of the lobes may be due to a combo of host motion wrt the IGM and the fact that one jet (the SE one) may have had to go through at least part of a neighboring galaxy's ISM (or maybe it's the other way round; the SE galaxy is the host and the NE jet is the one that had a tough time?).
Zsp 0.160 SDSS J233331.02+092534.8 may the host, despite its spectrum having no hint of an AGN:
But maybe the bigger-looking neighbor, SDSS J233331.31+092533.1, is the host (it has no SDSS spectrum)?
Of course, we're seeing these galaxies in projection, so we don't know what their physical separation actually is ...
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by ChrisMolloy in response to JeanTate's comment.
Here's an overlay. Any chance this is a #hybrid? Both possible hosts above have ALLWISE references also.
The contour overlay image in this post was created from sources, and using methods, described in this RGZ Talk
thread.Posted
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by Dolorous_Edd
Any chance this is a #hybrid
I don't think so, more like a wat
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by ivywong scientist, admin
I agree, there isn't a clear hot spot on one side.. so this is likely a #wat
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