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SUZAKU VIEW OF POWERFUL GAMMA-RAY QUASARS

机译:SUZAKU强大的γ射线拟态视图

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摘要

We present the results from multiwavelength campaigns of three powerful gamma-ray quasars, PKS 1510-089, RBS 315 and Swift J0746.3+2548, recently organized with Suzaku. The Suzaku observation provided one of the highest S/N X-ray spectra ever reported between 0.3 and 50 keV. For these quasars, the X-ray spectrum is well represented by an extremely hard power-law with photon index Gamma similar or equal to 1.2, but is augmented by an additional soft component apparently below 1 keV for PKS 1510-089, whereas a strong deficit of soft photons is observed in RBS 315. We model the broadband spectra of these powerful quasars and argue that the power of the jet is dominated by protons but with the number of electrons/positrons exceeding the number of protons by a factor similar or equal to 10. We also argue that an extremely hard X-ray spectra may result from a double power-law form of the injected electrons, with the break energy gamma br similar or equal to 1000 corresponding to the anticipated threshold of diffusive shock acceleration.
机译:我们介绍了最近与Suzaku合作组织的三个强大的伽玛射线类星体(PKS 1510-089,RBS 315和Swift J0746.3 + 2548)的多波长运动的结果。朱雀的观测提供了有史以来最高的S / N X射线光谱之一,据报道在0.3至50 keV之间。对于这些类星体,X射线光谱可以很好地表示为具有等于或等于1.2的光子指数Gamma的极硬幂律,但对于PKS 1510-089,显然可以通过低于1 keV的附加软成分来增强X射线光谱。在RBS 315中观察到了软光子的缺陷。我们对这些强大的类星体的宽带光谱进行了建模,并认为射流的功率由质子控制,但电子/正电子的数量超过质子的数量相近或相等。到10。我们还认为,注入的电子的双幂律形式可能会产生极硬的X射线光谱,其断裂能γbr类似于或等于1000,对应于预期的扩散冲击加速度阈值。

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