When certain stars collapse, they release overwhelmingblasts of energy called gamma-ray bursts ? the most powerful explosion in theuniverse. But the cosmic leftovers of these violent outbursts have been amystery ? until now.
Two new studies suggest that when gamma-raybursts explode, some can leave behind black holes like cosmic gravestones, whileothers may end up as spinning neutron stars.
In the ensuing dramatic collapse, a flood of high-energy,short-wavelength gamma-ray light is released. They are sometimes associatedwith supernovas ? another explosiveway stars die ? but are separate events.
"We have focused only on the brightest and most extremeGRBs, arguing that the energy release from these events is too large to bepowered by collapse to a neutron star (magnetar)," said study member BradCenko, a post-doctoral fellow from the University of California, Berkeley.
Magnetars are a type of neutronstar ? an object so dense its protons and electrons have merged toform neutrons. They are fast-spinning stars with extremely powerful magneticfields.
This team used data from NASA'sFermi spacecraft, which also observes in gamma-ray light.
The two studies, both presented Wednesday at the Gamma RayBursts 2010 conference in Annapolis, Md., help clarify the story behind some ofthe universe's most violent events. The scientists said their findings don'tconflict with each other.
"Our results are certainly not mutually exclusive - weboth are looking at relatively small sub-samples of GRBs," Cenko told SPACE.com.
Another group of scientists studied a sampling of gamma-raybursts observed by NASA's Swift gamma-ray satellite.
They found that 11 of the gamma-ray bursts bore particularsignatures in the pattern of light they emitted that suggested a magnetarwas present.
Some researchers had thought magnetars wouldn't be massiveenough to produce the kind of energy required for a gamma-ray burst. But thenew study suggests that at least some are.
"I think what our work shows is that magnetars are aviable model," said Paul O'Brien of the U.K.'s University of Leicester, amember of the research team. "For this feature that we see, it's very hardto see how you could do it for a black hole. It's much more consistent with amagnetar model."
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