Not exact matches
If astronomers act quickly, they can turn other instruments toward the point of origin and record a rapidly fading
afterglow of x-rays, visible light and
radio waves.
As the wave expands and the fire fades, the
afterglow changes «color» from x-ray to optical light to
radio waves.
Using
radio telescopes in Australia and optical telescopes in Hawaii, Keane and his colleagues detected an FRB and linked its fading
afterglow to a host galaxy some six billion light - years from Earth.
Instead they found a persistent
radio source whose strength varied randomly by a factor of three, often reaching levels that matched the initial brightness of the claimed
afterglow.
«Fast
radio burst «
afterglow» was actually a flickering black hole.»
Last February a team of astronomers reported detecting an
afterglow from a mysterious event called a fast
radio burst, which would pinpoint the precise position of the burst's origin, a longstanding goal in studies of these mysterious events.
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.
They also discovered that a monthlong
afterglow followed the event that could be observed with instruments used to detect optical frequencies, x-rays or
radio waves.
Their ultraviolet light reached free hydrogen gas in the surrounding regions, interacting with the atoms in a way that left a key signature in the
radio spectrum from the
afterglow of the Big Bang.
The researchers used
radio telescopes at the South Pole to stare at the cosmic microwave background radiation — a faint
afterglow left over from the big bang that permeates the universe.
«Sure enough, the
afterglow turned out to be brighter in the X-ray wavelengths, just as it was in the
radio.»
First limits on the very - high energy gamma - ray
afterglow emission of a fast
radio burst.
After the gamma - ray signal disappears, these GRBs exhibit «
afterglows» of x-rays, visible light, and
radio waves.
However, X-ray, optical and
radio emission continues in an «
afterglow.»
While the burst's
afterglow showed a steady decline in brightness at both optical and X-ray wavelengths, that was not the case at
radio wavelengths.
The X-ray observations disfavor simple top - hat jets and support the scenario where both the X-ray and
radio emissions are the
afterglow of an outflow or structured jet.