GAMMA-RAY AND X-RAY EMISSION FROM GAMMA-RAY-LOUD BLAZARS
Zhang Xiong (张雄)ab, Zhao Gang (赵刚)a, Xie Guang-zhong (谢光中)c, Zheng Guang-sheng (郑广生)d, Zhang Li (张力)d
a Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China; b Department of Physics, Yunnan Normal University, Kunming 650092, China; c Yunnan Observatory, Chinese Academy of Sciences, Kunming 650091, China; d Department of Physics, the University of Hong Kong, Hong Kong, China
Abstract We present a strong correlation of the gamma-ray (above 100 MeV) mean spectral indices $\alpha_\gamma$ and X-ray (1 keV) mean spectral indices $\alpha$X for 34 gamma-ray-loud blazars (16 BL Lac objects and 18 flat spectrum radio quasars). A strong correlation is also found between the gamma-ray flux densities $F_\gamma$ and X-ray flux densities FX in the low state for 47 blazars (17 BL Lac and 30 flat spectrum radio quasars). Possible correlation on the gamma-ray emission mechanism is discussed. We suggest that the main gamma-ray radiation mechanism is probably the synchrotron process. The gamma-ray emission may be somewhat different from that of BL Lac objects and flat spectrum radio quasars.
Received: 10 July 2000
Revised: 14 January 2001
Accepted manuscript online:
PACS:
98.54.Cm
(Active and peculiar galaxies and related systems (including BL Lacertae objects, blazars, Seyfert galaxies, Markarian galaxies, and active galactic nuclei))
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