ARG0001mrt, x-shaped lobes, more than one host and emission?
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by ChrisMolloy
Here's ARG0001mrt, which appears to be an #unusual emission. In terms of morphology, it appears #x-shaped, possibly a #triple or #doublelobe, a #wat, #overlapping lobes, and or one or more emissions. The contour overlays below are centred on SDSS J133437.35+313617.4, which is SSW of the ARG co-ordinates listed left.
The contour overlay image in this post was created from sources, and using methods, described in this RGZ Talk
thread. First in red.A possible host for some of the emission could be SDSS J133437.35+313617.4, which has a z_ph=0.182 ± 0.0311. This object has radio references in NED, and an ALLWISE reference, ALLWISE J133437.35+313617.3. This galaxy is SW of the centre of the emission.
There is a radio reference in NED for SDSS J133439.31+313618.5, which has a z_sp=0.196 +/-0.00003. This object has an ALLWISE reference, ALLWISE J133439.33+313618.3. This galaxy is positioned ESE of the centre of the lobes.
There are a number of other radio references in NED and SIMBAD for these lobes, but what could be a host or hosts is hard to determine. As per the ARG comments left, this could be an
unstudied, WAT or relic-type src?
In terms or morphology, it could also be a #doublelobe or #triple along the SW and NE axis, and maybe a #doublelobe or #triple along the W to E axis, but again. this is hard to ascertain. Also, this ARG field appears to be in a #cluster environment.
Here's a VLASS contour for comparison.
The contour overlay image in this post was created from sources, and using methods, described in this RGZ Talk
thread. VLASS in yellow.And for completeness, here's a First Wise Band 1 contour overlay.
The contour overlay image in this post was created from sources, and using methods, described in this RGZ Talk
thread. First contours in red, Wise Band 1 lime green.As always, comments, suggestions, welcome.
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by JeanTate
Apart from SDSS J133439.31+313618.5 being a (the?) likely host, there's not much that's clear for this #weird source. Obviously near the center of a rich, dense cluster of galaxies, so perhaps the complicated IGM (inter-galactic medium) is partly responsible? And the ISM (inter-stellar medium) of at least one galaxy too (SDSS J133437.35+313617.4), if it's foreground to the radio emission.
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