作者: R Buehler , JD Scargle , RD Blandford , Luca Baldini , MG Baring
DOI: 10.1088/0004-637X/749/1/26
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摘要: The Large Area Telescope on board the Fermi satellite observed a gamma-ray flare in Crab Nebula lasting for approximately nine days April of 2011. source, which at optical wavelengths has size 11 lt-yr across, doubled its flux within eight hours. peak photon was (186 ± 6) × 10–7 cm–2 s–1 above 100 MeV, corresponds to 30-fold increase compared average value. During flare, new component emerged spectral energy distribution, peaked an (375 26) MeV maximum. observations imply that emission region likely relativistically beamed toward us and variations motion are responsible variability.