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首页> 外文期刊>The Astrophysical journal >EGRET OBSERVATIONS OF THE 1993 MARCH GAMMA-RAY FLARE FROM PKS 0528 + 134
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EGRET OBSERVATIONS OF THE 1993 MARCH GAMMA-RAY FLARE FROM PKS 0528 + 134

机译:来自PKS 0528 + 134的1993年3月伽马射线耀斑的废气观察

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摘要

EGRET observation of PKS 0528 +134 during the 1993 March flare in gamma-rays is presented here. During the flare gamma-rays were detected at a level approximately three times greater than the observed intensity in earlier observations. Spectra of the source during the flare, as well as during the nonflaring state are presented. The flux history of PKS 0528 + 134 as observed from the start of the Compton Gamma Ray Observatory (CGRO) mission up to the end of Phase 3 (1993 October) is given. Multiwavelength observations of PKS 0528 + 134 during the flare are also presented. A detailed rela-tivistic SSC jet model agrees well with the 1993 March Multiwavelength spectrum; the data, however, are insufficient to discriminate between this and other emission models.
机译:这里介绍了在1993年3月耀斑期间EKET对PKS 0528 +134的EGR观测。在耀斑期间,探测到的伽玛射线水平大约是先前观察中观察到的强度的三倍。显示了在耀斑期间以及在非耀斑状态下光源的光谱。给出了从康普顿伽玛射线天文台(CGRO)任务开始到第三阶段结束(1993年10月)为止所观测到的PKS 0528 + 134的通量历史。还介绍了耀斑期间PKS 0528 + 134的多波长观测。详尽的相对论SSC射流模型与1993年3月的多波长光谱非常吻合。但是,数据不足以区分此排放模型和其他排放模型。

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