than typical stars in our neighborhood,
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, the LIGO team reports February 11 in the Astrophysical Journal Letters. ,
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?
One possibility is that the stars formed early in the universe before heavy elements had a chance to accumulate. At the other extreme, the stars could have formed more recently in a relatively nearby (or local) and pristine pocket such as a dwarf galaxy. “With one observation, it’s impossible to say if it’s on one side of the continuum or the other,
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,” says Vicky Kalogera,
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, a LIGO astrophysicist at Northwestern University in Evanston,
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, Ill.
The best estimates put the collision in a galaxy about 1.3 billion light-years away (give or take a few hundred million light-years) in the southern sky, roughly in the direction of the Magellanic Clouds,
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, two satellites of the Milky Way. A third LIGO facility, such as one proposed for India, will help narrow down precise positions of future detections. So would a simultaneous burst of electromagnetic radiation from the location of a collision. LIGO has agreements with telescopes around the world (and in space) to keep an eye out for any flashes of light that occur at the same time as a gravity wave detection. For LIGO’s debut,
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, no observatories reported anything definitive. But the Fermi gamma-ray satellite did see something interesting,
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, astrophysicist Valerie Connaughton and colleagues report online February 14 at arXiv.org.
“We found a little blip that’s weaker than anything we’d normally look at,” says Connaughton, of the Universities Space Research Association in Huntsville, Ala. At 0.4 seconds

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