«A repeating fast
radio burst from an extreme environment: Extragalactic source of radio - wave flashes resides in a powerfully magnetized astrophysical region.»
The observations by the Breakthrough Listen team at UC Berkeley using the Robert C. Byrd Green Bank Telescope in West Virginia show that the fast
radio bursts from this object, called FRB 121102, are nearly 100 percent linearly polarized, an indication that the source of the bursts is embedded in strong magnetic fields like those around a massive black hole.
MYSTERIOUS
radio bursts from the distant cosmos are revealing their true nature.
For a decade, astronomers have puzzled over ephemeral but incredibly powerful
radio bursts from space.
Five new fast
radio bursts from the HTRU high - latitude survey at Parkes: first evidence of two - component bursts.
Not exact matches
The number of wave crests arriving
from Fast
Radio Bursts per second — their «frequency» — is in the same range as that of radio sig
Radio Bursts per second — their «frequency» — is in the same range as that of
radio sig
radio signals.
MeerLICHT, a 65 - centimeter optical telescope, is expected to help identify the sources of fast
radio bursts (FRBs)-- extremely brief, energetic flashes of
radio waves
from remote galaxies.
A class of odd
radio bursts first detected by the Parkes telescope years ago came
from an advanced civilization — if advanced means people on Earth so eager for a microwaved meal they open the oven before the beep.
And the gamma - ray emission
from FRB 131104 outshines its
radio emissions by more than a billion times, dramatically raising estimates of the
burst's energy requirements and suggesting severe consequences for the
burst's surroundings and host galaxy.
Discovery of the gamma - ray «bang»
from FRB 131104, the first non-
radio counterpart to any FRB, was made possible by NASA's Earth - orbiting Swift satellite, which was observing the exact part of the sky where FRB 131104 occurred as the
burst was detected by the Parkes Observatory
radio telescope in Parkes, Australia.
TWISTS AND TURNS The twisted waves
from a distant fast
radio burst suggest the
burst originates
from a neighborhood with a strong magnetic field.
An unknown object that appears close to an expanding cloud of matter
from a supernova (top) spat out five strong
radio bursts in 2002 (bottom).
OXON HILL, Md. — Fast
radio bursts could come
from a turbulent home.
Radio telescopes have picked up intense
bursts of low - frequency static
from a mysterious source that may lie hidden near the center of our Milky Way galaxy.
The team measured the
radio waves
from 16 distinct
bursts over three two - hour observational runs spanning several months.
Questions remain about whether all fast
radio bursts, including the ones that don't repeat, come
from such exciting neighborhoods.
The change in the
burst's brightness appears to be exactly the same at
radio and optical frequencies; this can happen, say Garnavich and his collaborators Avi Loeb and Kris Stanek
from the Center for Astrophysics in Cambridge, Massachusetts, only if part of the expanding ring passed behind a star located exactly between Earth and the ring itself.
«The discovery of a repeating FRB has not only narrowed down the possible astrophysical origins of FRBs,» says lead author Laura Spitler of the Max Planck Institute for
Radio Astronomy in Bonn, Germany, «but we also have a better shot at unraveling their nature by being able to observe more
bursts from this source.»
Mega
bursts of
radio waves that seem to come
from a galaxy far, far away have a weird pattern — here's what you need to know
Combined with the fact that
bursts seem to evolve
from energetic gamma rays to X-rays to visible light, which means they cool off over time, the
radio data supported the idea that they are huge fireballs, expanding at near - light - speed and cooling as they go.
An armada of space observatories measured gamma rays
from the
burst, while
radio telescopes on Earth helped pinpoint the source of the activity.
Fast
radio bursts, which flash for just a few milliseconds, created a stir among astronomers because they seemed to be coming
from outside our galaxy, which means they would have to be very powerful to be seen
from Earth, and because none of those first observed were ever seen again.
These
bursts of
radio waves have remained a mystery since the first one was discovered in 2007 by researchers scouring archived data from Australia's Parkes Radio Telescope in search of new pul
radio waves have remained a mystery since the first one was discovered in 2007 by researchers scouring archived data
from Australia's Parkes
Radio Telescope in search of new pul
Radio Telescope in search of new pulsars.
One of the rare and brief
bursts of cosmic
radio waves that have puzzled astronomers since they were first detected nearly 10 years ago has finally been tied to a source: an older dwarf galaxy more than 3 billion light years
from Earth.
This detection follows 11 previously recorded outbursts of
radio waves
from the same location, the only known repeater in a class of enigmatic eruptions known as fast
radio bursts.
The continuing barrage
from this repeating source, roughly 3 billion light - years away in the constellation Auriga, implies that whatever is causing some
radio bursts is not a one - time destructive
Anthony Readhead of the Owens Valley
Radio Observatory at Caltech and colleagues caught two small, hot
bursts traveling away
from a bright galaxy called J1415 +1320 at near the speed of light.
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.
Dark matter hitting black holes could be the source of some fast
radio bursts — mysterious blasts of
radio waves that come
from billions of light years away, first detected 10 years ago.
A team studying data
from a recent sky survey has spotted a huge
burst of
radio waves that came and went in the blink of an eye and has not returned since.
A rapid and powerful
burst of
radio waves is found through an analysis of archival pulsar data, suggestive of a new class of
radio bursts, perhaps
from a supernova.
New detections of
radio waves
from a repeating fast
radio burst have revealed an astonishingly potent magnetic field in the source's environment, indicating that it is situated near a massive black hole or within a nebula of unprecedented power.
Breakthrough Listen allotted tens of hours of observational time on the Green Bank Telescope to recording
radio emissions
from FRB 121102, and last August 26 detected 15
bursts over a relatively short period of five hours.
Because
radio signals travel faster than particles, the completed e-CALLISTO can also work as an early - warning system for
radio bursts, alerting space mission control centres to upcoming disturbances caused by coronal mass ejections
from the Sun.
The Dutch and Breakthrough Listen teams suggest that the fast
radio bursts may come
from a highly magnetized rotating neutron star — a magnetar — in the vicinity of a massive black hole that is still growing as gas and dust fall into it.
Fast
radio bursts are brief, bright pulses of
radio emission
from distant but so far unknown sources, and FRB 121102 is the only one known to repeat: more than 200 high - energy
bursts have been observed coming
from this source, which is located in a dwarf galaxy about 3 billion light years
from Earth.
The nearly 100 percent polarization of the
radio bursts is unusual, and has only been seen in
radio emissions
from the extreme magnetic environments around massive black holes, such as those at the centers of galaxies.
Banking that she'd spot a «live»
burst, Petroff had an international team poised to make rapid follow - up observations, at wavelengths
from radio to X-rays.
The repeating
bursts from this object, named FRB 121102 after the date of the initial
burst, allowed astronomers to watch for it using the National Science Foundation's (NSF) Karl G. Jansky Very Large Array (VLA), a multi-antenna
radio telescope system with the resolving power, or ability to see fine detail, needed to precisely determine the object's location in the sky.
These fast
radio bursts (FRBs) are brief, bright pulses of
radio emission
from distant but unknown sources.
In addition to detecting the bright
bursts from FRB 121102, the VLA observations also revealed an ongoing, persistent source of weaker
radio emission in the same region.
Radar pulses (short
bursts of
radio - frequency energy) emitted
from a ground - based transmitter are reflected by a meteor's trail.
One fun bit of synchronicity: I met a
radio astronomer
from the Netherlands, and she uses Breakthrough Listen data to search for fast
radio bursts, or FRBs.
They are also developing (with Dr. Kent Wood of NRL) a model that attempts to account for the
radio bursts as a new type of outburst
from a class of sources known as «magnetars.»
They also plan to keep monitoring the steady
radio emission
from the vicinity of the Spitler
burst to see if its properties change in time, as expected based on that theory.
The phenomena, known as fast
radio bursts or FRBs, were first detected in 2007 by astronomers scouring archival data
from Australia's Parkes Telescope, a 64 - meter diameter dish best known for its role receiving live televison images
from the Apollo 11 moon landing in 1969.
And, according to Laura Spitler, namesake of the Spitler
burst and a researcher at the Max Planck Institute for
Radio Astronomy, in Bonn, Germany, magnetars generally form
from stellar explosions called Type - I superluminous supernovas.
A team of astronomers using a pair of National Science Foundation
radio telescopes has made the first measurements of the size and expansion of a mysterious, intense fireball resulting
from a cosmic gamma ray
burst last May.
Astronomers have used the National Science Foundation's Very Large Array
radio telescope to make the first detection of
radio emission
from a cosmic gamma - ray
burst.