Different pattern

• by akil_hashim

  A very different pattern than most.

  Posted September 15, 2014 5:56 AM

• by 42jkb scientist, admin in response to akil hashim's comment.

  This would be considered to be #bent and a black hole group (#bhgroup).

  Posted September 15, 2014 6:42 AM

• by JeanTate

  Centered on SDSS J135142.13+555943.1, z_ph 0.091±0.0132/0.090±0.0189, SDSS looks like this:

  

  How do the galaxies map to the radio emissions? Specifically, which galaxy is the host of what radio emission?

  

  Boilerplate: SDSS image per http://skyservice.pha.jhu.edu/DR10/ImgCutout/getjpeg.aspx, FIRST (red) contours derived from the FITS file produced using SkyView with Python code described in this RGZ Talk thread. Image center (J2000.0) is the galaxy [); "z_ph" its SDSS photometric redshift.

  Posted September 17, 2014 1:13 AM

• by 42jkb scientist, admin in response to JeanTate's comment.

  We would require higher resolution radio observations to determine how the radio emission maps to the galaxies in the group. I would say that the main active black hole is the central elliptical though.

  Posted September 18, 2014 6:41 AM