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Transient optical emission from the error box of the γ-ray burst of 28 February 1997
Transient optical emission from the error box of the γ-ray burst of 28 February 1997
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Transient optical emission from the error box of the γ-ray burst of 28 February 1997
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Transient optical emission from the error box of the γ-ray burst of 28 February 1997
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Transient optical emission from the error box of the γ-ray burst of 28 February 1997
Transient optical emission from the error box of the γ-ray burst of 28 February 1997
Journal Article

Transient optical emission from the error box of the γ-ray burst of 28 February 1997

1997
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Overview
For almost a quarter of a century 1 , the origin of γ-ray bursts— brief, energetic bursts of high-energy photons—has remained unknown. The detection of a counterpart at another wavelength has long been thought to be a key to understanding the nature of these bursts (see, for example, ref. 2), but intensive searches have not revealed such a counterpart. The distribution and properties of the bursts 3 are explained naturally if they lie at cosmological distances (a few Gpc) 4 , but there is a countervailing view that they are relatively local objects 5 , perhaps distributed in a very large halo around our Galaxy. Here we report the detection of a transient and fading optical source in the error box associated with the burst GRB970228, less than 21 hours after the burst 6,7 . The optical transient appears to be associated with a faint galaxy 7,8 , suggesting that the burst occurred in that galaxy and thus that γ-ray bursts in general lie at cosmological distance.