NGC 4061 has two radio jets that appear to be very straight and that dramatically oppose each other. At a distance of 26,000 ly (8 kpc) from the core the jets appear to suddenly sweep back. This sudden bending of the jets suggest that they are leaving theinterstellar medium (ISM) of NGC 4061 and entering into theintracluster medium (ICM). After the sharp bending, the jets continue to open for about 82,000 ly (25 kpc) and extend into a "U" or horseshoe morphology similar toNGC 1265, with each jet having a length of 160,000 ly (50 kpc). This morphology is thought to be due to the motion of NGC 4061 through the ICM with sufficient velocity to bend the jets byram-pressure stripping.[15]
The interaction withNGC 4065 may have also contributed to bending the jets.[9]
On February 18, 2008 atype Ia supernova designated as SN 2008bf was discovered in NGC 4061.[24][25][26][27] However, the Open Supernova Catalog suggests that the host galaxy may be the nearbyNGC 4065.[27]
1.^ This was determined by multiplying the given scale length in the paper of 0.55arcseconds=820 ly (250 pc) by 9.1 to get the diameter of the dust disk.
^abBurns, Jack O.; Hanisch, Robert J.; White, Richard A.; Nelson, Eric R.; Morrisette, Kim A.; Moody, J. Ward (1987-09-01). "A VLA 20 CM survey of poor groups of galaxies".The Astronomical Journal.94:587–617.Bibcode:1987AJ.....94..587B.doi:10.1086/114494.ISSN0004-6256.
^Zaninetti, Lorenzo (2009-03-06). "A turbulent model for the surface brightness of extragalactic jets".Revista Mexicana de Astronomía y Astrofísica.45:25–53.arXiv:0903.1170.Bibcode:2009RMxAA..45...25Z.
^Pinkney, J. C.; Nuker Team (2005-05-01). "Kinematics and Black Hole Mass for the Narrow-Angle Tailed Radio Galaxy NGC 4061".American Astronomical Society Meeting Abstracts #206.206: 11.17.Bibcode:2005AAS...206.1117P.