Letters to Nature

Nature 404, 363-365 (23 March 2000) | doi:10.1038/35006001; Received 8 October 1999; Accepted 5 January 2000

Discovery of a new population of high-energy big gamma-ray sources in the Milky Way

N. Gehrels, D. J. Macomb, D. L. Bertsch, D. J. Thompson and R. C. Hartman

  1. Laboratory for High Energy Astrophysics, NASA's Goddard Space Flight Centre, Greenbelt, Maryland 20771, USA

Correspondence to: N. Gehrels Correspondence and requests for materials should be addressed to N. G. (e-mail: Email: gehrels@gsfc.nasa.gov).

One of the great mysteries of the high-energy gamma-ray sky is the group of approx170 unidentified point sources1, 2 found along the Galactic plane. They are more numerous than all other high-energy gamma-ray sources combined and, despite 20 years of effort, no clear counterparts have been found at other wavelengths. Here we report a new population of such objects. A cluster of approx20 faint sources appears north of the Galactic Centre, which is part of a broader class of faint objects at mid-latitudes. In addition, we show in a model-independent way that the mid-latitude sources are distinct from the population of bright unidentified sources along the Galactic plane. The distribution on the sky indicates that the faint mid-latitude sources are associated with the Gould belt3, 4 of massive stars and gas clouds at approx600 light years distance, as has been previously suggested5.

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