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首页> 外文期刊>The Astrophysical journal >EGRET GAMMA-RAY SOURCES: GRO J0744 + 54 AND GRO J0957 + 65 ( = BL LACERTAE OBJECT 0954 + 658)
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EGRET GAMMA-RAY SOURCES: GRO J0744 + 54 AND GRO J0957 + 65 ( = BL LACERTAE OBJECT 0954 + 658)

机译:EGR伽玛射线源:GRO J0744 + 54和GRO J0957 + 65(= BL LACERTAE OBJECT 0954 + 658)

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摘要

EGRET detected an unidentified source, GRO J0744 + 54, at a significance of 6.5 σ, during its observations from 1993 June 28 to July 12. The source was seen again in the following 2 week viewing period and was weakly evident in the earlier phase 1 of the EGRET observations. Considering the variability of its gamma-ray flux, and its location at high Galactic latitude, GRO J0744 + 54 is likely to be a previously undetected blazar. Its most likely identification is with the radio source 87GB 073840.5 + 545138. A second source, GRO J0957 + 65, was seen by EGRET during the same two viewing periods at a combined significance of 5.7 σ. The most probable counterpart of GRO J0957 + 65 is the BL Lacertae object 0954 + 658. The spectra, time variability, and positions of the two sources are presented. Multiwavelength observations of 0954 + 658 are also presented.
机译:EGRET在1993年6月28日至7月12日的观测中,发现了一个未识别的源GRO J0744 + 54,其显着性为6.5σ。在接下来的2周观察期中再次看到该源,在早期1期中该信号较弱。 EGRET观察结果。考虑到其伽马射线通量的可变性以及其在高银纬度上的位置,GRO J0744 + 54可能是以前未发现的大隐身。它最有可能的标识是87GB 073840.5 + 545138无线电源。在相同的两个观看时间段内,EGRET观察到了第二个源GRO J0957 + 65,其综合有效值为5.7σ。 GRO J0957 + 65的最可能对应物是BL Lacertae对象0954 +658。显示了这两个源的光谱,时间可变性和位置。还介绍了0954 + 658的多波长观测结果。

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