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parameter Relativistic wave
equations Sparks, W. B.; et al. (1992). "A
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- 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...
- ± 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...
-
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...
- 000
light years points to the
upper left in the image, with a
shorter "
counterjet"
aimed in the
opposite direction. In this image, low-energy X-rays are...
-
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...
