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Magnetic Explosions In The Distant Universe Get The Gamma Going

Gamma-ray bursts are thought to be the most powerful explosions in the Universe, yet the cause of these high-energy flashes remains a mystery. Blindingly bright for space-based gamma-ray detectors the burst sources are so faint at visible wavelengths that large telescopes and sensitive cameras are required to search for them. The faint optical flash from a relatively intense gamma-ray burst detected on December 14th of last year seems to have originated in the galaxy indicated in this Hubble Space Telescope image - taken months after the burst had faded from view. Astronomers have recently announced that this galaxy's spectrum, recorded using the large Keck telescope atop Hawaii's Mauna Kea, indicates that it lies at a distance of about 12 billion light-years. The energy required to produce the observed flash of gamma-rays from this distance would be staggering! Some estimates suggest that in a few seconds the burster released the equivalent energy of several hundred supernovae (exploding stars). The eruption of such a large amount of energy in such a short time is so extreme that even exotic theoretical models of the bursters are being challenged. Could the bursts be caused by the cataclysmic merger of neutron stars with black holes ... or something as yet unknown? Credit: S. R. Kulkarni, S. G. Djorgovski (Caltech), the Caltech GRB Team , NASA.
by Staff Writers
London UK (SPX) Feb 12, 2007
Long duration gamma-ray bursts (GRBs), first discovered in the 1970s, are the most explosive events in the Universe. Finding out what happens during these cataclysmic events is a major challenge, partly because they usually occur at the edge of the visible Universe and partly because the bursts last only a matter of seconds.

Observations accumulated over the last decade have led to a consensus that at least some GRBs mark the death throes of a giant star as its core collapses to form a black hole. Until now, it has generally been thought that the black hole ejects a jet of plasma (extremely hot gas) which is blasted outwards at close to the speed of light.

This theory is called into question by a new study led by Pawan Kumar from the University of Texas. The work has been accepted for publication in the journal, "Monthly Notices of the Royal Astronomical Society".

Magnetic Outflow
Scientists have long speculated that the gamma-ray emission we see comes from fluctuations in the speed of the ejected material. The faster and slower ejecta collide, producing shocks in the jet which result in the emission of gamma-rays. Although this internal shock model is the standard explanation, it relies on the jet consisting of ordinary matter -- the same sort of material that we are made from -- or what scientists call baryons.

Now, however, Pawan Kumar and colleagues have cast doubt on this model. Instead of the GRBs being generated by internal shocks, Kumar's team finds that the jet is actually a powerful magnetic outflow which transports huge amounts of energy away from the collapsed star.

Using data from the Swift satellite, Professor Kumar's team has analysed a sample of 10 gamma-ray bursts that were recorded between January 2005 and May 2006. In each case, Swift collected gamma-ray, X-ray and optical light immediately after the explosions were detected. Such multi-wavelength observations are essential if the researchers are to understand what happens after the brief burst fades and the source object is only visible in X-rays or visible light.

"Swift is uniquely capable of such simultaneous multi-wavelength observations," said Neil Gehrels of NASA's Goddard Space Flight Center, Principal Investigator for the Swift satellite.

The new study reveals the physical process responsible for the generation of gamma-ray radiation and the distance from the black hole where this radiation is produced.

"The gamma-ray source is located about 10 billion km from the black hole, or 100 times further than previously thought," said Professor Kumar. "This and several other lines of evidence put forward in our work suggest that the outflow is dominated by the magnetic field."

The data indicate that a magnetic jet decays into gamma-rays. The subsequent interaction (of the jet) with the surrounding gas causes intense heating and this produces an afterglow that is seen at X-ray and visible light wavelengths.

Dr. Paul O'Brien from the University of Leicester, a co-investigator on the project, said, "In just a few seconds gamma-ray bursts emit as much energy as the Sun does in 10 billion years. The Swift observations are telling us that this emission is due to an outflow in which magnetic fields transport the energy. If confirmed, this will alter our view of how these objects work."

"Using the Swift data we can accurately measure the times when the prompt emission stops and the afterglow becomes visible," said Richard Willingale, also from the University of Leicester. "These times constrain the distance of the emitting region from the black hole and hence the physical processes involved."

Since its launch on 20 November 2004, Swift has observed over 200 gamma-ray bursts and provides prompt data on almost all of them.

"Swift can turn and observe a gamma-ray burst with its X-ray and optical telescopes in just a few tens of seconds," said Professor David Burrows from Pennsylvania State University, lead investigator for the X-ray telescope on Swift. "This capability allows us to capture a snapshot of the early emission which carries information on the physical processes involved."

Dr Silvia Zane, from the Mullard Space Science Laboratory said, "This is going to revolutionise our understanding of the cause of such explosions."

Related Links
RAS
Swift at Leicester
Swift at Goddard
Swift significant observations
Swift Observes an Unusual Bang in the Far Universe
Gamma ray bursts
Animation of exploding stars
Stellar Chemistry, The Universe And All Within It
Stellar Chemistry, The Universe And All Within It



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The Dark Side Of Nature Makes For Almost A Perfect Crime
Paris, France (ESO) Jan 03, 2007
Nature has again thrown astronomers for a loop. Just when they thought they understood how gamma-ray bursts formed, they have uncovered what appears to be evidence for a new kind of cosmic explosion. These seem to arise when a newly born black hole swallows most of the matter from its doomed parent star.







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