ARG00023hz IS SDSS J153143.46+240419.1 CENTER IS IT THE RADIO SOURCE GALAXY?
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by 1001G
Z 0.096 3C 321 SDSS J153143.46+240419.1 CENTER IT SEEMS TO FIT NVSS IMAGE IS IT THE RADIO SOURCE GALAXY?
SOUTH Z 0.271 SDSS J153143.81+240412.1 GALAXY.
NORTH SDSS J153143.30+240421.1 GALAXY.SDSS J153143.46+240419.1
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by JeanTate
Added to the list ...
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by zutopian
PKS0347+05: a radio-loud/radio-quiet double AGN system triggered in a major galaxy merger
C. Tadhunter, C. Ramos Almeida, R. Morganti, J. Holt, M. Rose, D. Dicken, K. InskipWe present optical, infrared and radio observations of the powerful FRII radio source PKS0347+05 (z=0.3390), and demonstrate that it is a rare example of a radio-loud/radio-quiet double AGN system, comprising a weak line radio galaxy (WLRG) separated by 25 kpc (in projection) from a Seyfert 1 nucleus at the same redshift. (...)
(Submitted on 17 Sep 2012)
http://arxiv.org/abs/1209.3568Posted
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by zutopian
Further Radio Zoo images of this jet.:
http://radiotalk.galaxyzoo.org/#/subjects/ARG00023hv same as: http://radiotalk.galaxyzoo.org/#/subjects/ARG00023hx
http://radiotalk.galaxyzoo.org/#/subjects/ARG00023f5 same as: http://radiotalk.galaxyzoo.org/#/subjects/ARG00023ewIDs of the other lobe: ?
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by JeanTate in response to JeanTate's comment.
The SE lobe is indeed complex; is there an unrelated radio source lurking in it? A zoomed-in overlay, centered on that lobe, later!
The image in this post was created from sources, and using methods, described in this RGZ Talk post. The object at the center of the image is SDSS J153143.46+240419.1
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by JeanTate
A zoomed-in overlay, centered on that lobe, later!
Not sure this helps much; two versions, with different contour spacings:
Here's the apparent host, a STAR:
Per NED, an x-ray source (CXO J153150.6+240243) is just ~3" away, here (I've no idea what the error bars would be):
Perhaps this is a distant, very radio-bright source, viewed almost 'end-on', which just coincidentally happens to be close to the line of sight of a boring M star? And the fact that it's invisible in both IR and optical would make it an incredible #ifrs, no?
What do you think?
The image in this post was created from sources, and using methods, described in this RGZ Talk post. The object at the center of the image is SDSS J153150.42+240242.5
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