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- W1921631672 abstract "The vast majority of the high-energy γ-ray sources discovered by EGRET are still unidentified. Percentages range from 50% at high galactic latitudes, where blazars are responsible for almost all identified sources, to more than 90% near the galactic plane, where isolated neutron stars appear to be the only certified class of sources of high energy γ-rays. In spite of all the efforts devoted to the identification problem, the only success story, so far, appears to be the chase for Geminga, where X-rays led the way to eventual optical identification. Similar searches are now starting to produce encouraging results, although none has reached, as yet, a certified identification." @default.
- W1921631672 created "2016-06-24" @default.
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- W1921631672 date "2001-01-01" @default.
- W1921631672 modified "2023-10-18" @default.
- W1921631672 title "A multiwavelength strategy for identifying celestial γ-ray sources" @default.
- W1921631672 doi "https://doi.org/10.1063/1.1419477" @default.
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