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作 者:Yong-Yun Chen Xiong Zhang Ding-Rong Xiong Si-Ju Wang Xiao-Ling Yu
机构地区:[1]Department of Physics, Yunnan Normal University, Kunming 650500, China [2]Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China [3]Dongxing Middle School, Chuxiong 675000, China
出 处:《Research in Astronomy and Astrophysics》2016年第1期107-116,共10页天文和天体物理学研究(英文版)
基 金:the Science Foundation of Yunnan Province of China (Grant Nos.2012F13140 and 2010CD046);supported by the National Natural Science Foundation of China (Grant Nos.11063004,11163007 and U1231203);the High-Energy Astrophysics Science and Technology Innovation Team of Yunnan Higher School and Yunnan Gravitation Theory Innovation Team (2011c1);supported by the research innovation fund for graduate students,Yunnan Normal University (yjs201566)
摘 要:We study the γ-ray luminosity and beaming effect for Fermi blazars.Our results are as follows.(i) There are significant correlations between γ-ray luminosity and radio core luminosity,and between γ-ray luminosity and R_v,which suggests that the γ-ray emissions have a strong beaming effect,(ⅱ) Using the L_(ext)/M_(abs) as an indicator of environment effects,we find that there is no significant correlation betweenγ-ray luminosity and L_(ext)/M_(abs) for all sources when we remove the effect of redshift.Flat spectrum radio quasars considered alone also do not show a significant correlation,but BL Lacertae objects(BL Lacs) still show a significant correlation when we remove the effect of redshift.These results suggest that the γ-ray emission may be affected by the environment on a kiloparsec scale for BL Lacs.We study the γ-ray luminosity and beaming effect for Fermi blazars.Our results are as follows.(i) There are significant correlations between γ-ray luminosity and radio core luminosity,and between γ-ray luminosity and R_v,which suggests that the γ-ray emissions have a strong beaming effect,(ⅱ) Using the L_(ext)/M_(abs) as an indicator of environment effects,we find that there is no significant correlation betweenγ-ray luminosity and L_(ext)/M_(abs) for all sources when we remove the effect of redshift.Flat spectrum radio quasars considered alone also do not show a significant correlation,but BL Lacertae objects(BL Lacs) still show a significant correlation when we remove the effect of redshift.These results suggest that the γ-ray emission may be affected by the environment on a kiloparsec scale for BL Lacs.
关 键 词:BL Lacerate objects: general -- quasars: general -- gamma-rays: galaxies -- radio continuumgalaxies
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