The radio telescopes
showed the radio emission steadily gaining strength.
Not exact matches
The time evolving model
shows that the eastern (left) side of the expanding shock front expands more quickly than the other side, and generates more
radio emission than its weaker counterpart.
Rampadarath explains: «Comparing the VLA images at
radio wavelengths to Chandra's X-ray observations and the hydrogen -
emission detected by Hubble,
shows that features are not only connected, but that the
radio outflows are in fact the progenitors of the structures seen by Chandra and Hubble.
The X-ray data
show hot gas and the
radio data
show emission from electrons that have been accelerated to high energies by the nova shock wave.
They
show that as the plasma expands into the surrounding vacuum, the ions and electrons travel at different speeds and separate in a way that creates
radio frequency
emissions.
«Advancing technology has revealed more and more of the Universe to us over the past few decades, and our study
shows individual objects that account for about 96 percent of the background
radio emission coming from the distant Universe,» Condon said.
New research by Harvard astronomers Peter Williams and Edo Berger
shows that the
radio emission believed to be an afterglow actually originated from a distant galaxy's core and was unassociated with the fast
radio burst.
Observations of the shock between this pair of clusters
showed that the
radio emission was connected to the galaxy's jet, so clearly the electrons must have been initially accelerated by the black hole and then reaccelerated by the shock waves.
This
showed that the brown dwarf's
radio emission had risen to a strong peak, then weakened.
The object's core, near the orbiting pair of stars,
showed changes in the brightness of its
radio emission.
As
shown in our additional, composite image, part of the evidence for this heating process comes from the similarity in location between the hydrogen and X-ray
emission, both thought to be caused by shocks, and the
radio jets.
However, the original Green Bean population
show little to no
emission at
radio wavelengths.
Observations with
radio and infra - red telescopes
show that NGC 5128 swallowed a spiral galaxy probably about five hundred million years ago and the effects of the collision powers the strong
radio emission.
That same year, another team made an even more - detailed image of the region that
showed not only the mini-spiral but also a distinct, separate point of
radio emission corresponding to the exact center of the Galaxy.
From Australia,
radio host Vivien Langford of the 3 CR Beyond Zero
Emissions show, talks in studio with David Spratt, author of Code Red, plus union icon Colin Long and psychologist Lyn Bender.
In the Spring of 1994, scientists were observing an X-ray emitting object called GRS 1915 +105, which had just
shown an outburst of
radio emission.
And Pruitt recently told a conservative
radio talk
show host on August 9 that the Clean Air Act can not be used to regulate greenhouse gas
emissions.
A conservative author and
radio talk
show host, he didn't buy the notion that greenhouse - gas
emissions were causing temperatures to rise.
For example, when the bar chart
showed a 0 % cut in
emissions there were two
radio buttons corresponding to «Reduce
emissions by 0 %» and «Reduce
emissions by more».