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耀变体3C 454.3的能谱光变研究

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基于平谱射电类星体3C 454.3在2010-2016年间42个时段的光谱能量分布(SED)数据,利用单区均匀轻子模型得到了其光变参数,结果发现:(1)电子谱指数p1支持光变时的加速机制是斜激波加速;(2)辐射区位置在宽线区之外,尘埃环之内;(3)功率PB<Pr<Pe<Pp,Pp/Pjet=68.6%,说明喷流的大部分能量是由冷质子携带的;(4)均分参数ε大于1的比值为93%,意味着喷流以粒子为主导.
Study on the Energy Spectrum Variability of Blazar 3C 454.3
The single-zone homogeneous lepton model was used to fit the simultaneous SED data of the flat-spectrum radio quasar 3C 454.3 in 42 periods from 2010 to 2016.The distribution of various pa-rameters during the variability was given,and the acceleration mechanism and the location of the radia-tion region,peak luminosity and peak frequency,power of each component in the jet,and total power of the jet were analyzed.It is found that:(1)the electron spectral index p1 supports the acceleration mechanism of the shock acceleration during variability,(2)the radiation region is located outside the broad-line region and inside the dust tours,(3)PB<Pr<Pe<Pp and Pp/Pjet=68.6%indicate that most of the energy of the jet is carried by cold protons,and(4)the proportion of parameters with an average value of ε greater than 1 is 93%,indicating that particles dominate the jet.

3C 454.3VariabilitySED

施永有、谢照华、李国明、邓霄、宋雨洁、徐云冰

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云南师范大学物理与电子信息学院,云南 昆明 650500

3C 454.3 光变 SED

2024

云南师范大学学报(自然科学版)
云南师范大学

云南师范大学学报(自然科学版)

CSTPCD
影响因子:0.54
ISSN:1007-9793
年,卷(期):2024.44(6)