NGC 4061 has two radio jets that appear to be very straight and that dramatically oppose each other. At a distance of 26,000ly (8kpc) from the core the jets appear to suddenly sweep back. This sudden bending of the jets suggest that they are leaving the interstellar medium (ISM) of NGC 4061 and entering into the intracluster medium (ICM). After the sharp bending, the jets continue to open for about 82,000ly (25kpc) and extend into a "U" or horseshoe morphology similar to NGC 1265, with each jet having a length of 160,000ly (50kpc). This morphology is thought to be due to the motion of NGC 4061 through the ICM with sufficient velocity to bend the jets by ram-pressure stripping.[15]
The interaction with NGC 4065 may have also contributed to bending the jets.[9]
Dust Disk
NGC 4061 has a dust disk with a diameter of 7,420ly (2.275kpc).[21]
On February 18, 2008 a Type Ia supernova designated as SN 2008bf was discovered near NGC 4061.[24][25][26] However, the host galaxy may instead be the nearby NGC 4065.
1.^This was determined by multiplying the given scale length in the paper of 0.55 arcseconds=820ly (250pc) by 9.1 to get the diameter of the dust disk.
12Burns, 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.