- S2CID 90973. Meyer,
Eileen (June 2018). "Detection of an Optical/UV Jet/
Counterjet and
Multiple Spectral Components in M84". The
Astrophysical Journal. 680...
- W.B.; Fraix-Burnet, D.; Macchetto, F.; Owen, F.N. (February 1992). "A
counterjet in the
elliptical galaxy M87". Nature. 355 (6363): 804–806. Bibcode:1992Natur...
-
parameter Relativistic wave
equations Sparks, W. B.; et al. (1992). "A
counterjet in the
elliptical galaxy M87". Nature. 355 (6363): 804–806. Bibcode:1992Natur...
- S2CID 118034129. Meyer,
Eileen (June 2018). "Detection of an Optical/UV Jet/
Counterjet and
Multiple Spectral Components in M84". The
Astrophysical Journal. 680...
- component,
which is
bright in
optical wavelengths and a
redshifted faint counterjet. A
second pair of
bipolar jets,
called HH 121 was
discovered in the near-infrared...
-
third member. The jet
towards HH 1 is
visible in
optical images, but the
counterjet towards HH 2 was
detected in the
infrared with the
Spitzer Space Telescope...
-
connecting it.
There is also some lobe
luminosity located on the side of the
counterjet with the jet's side
having halo emission. The superm****ive
black hole...
- ± 0.02 M⊙
based on the MBH - MK correlation.
According to the jet to
counterjet brightness ratio, the
central ~ 10 kpc jet
region of NGC 6051 is potentially...
-
milliarcseconds (mas) but then
curves northwards. Hot
spots are
visible at the
counterjet direction in
radio images.
There is also a
faint halo. The jet has been...
-
outflow is bipolar, only one jet is
visible at
visual wavelengths. The
counterjet is
invisible as it is
moving away from
Earth into the dark
cloud that...
