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国家自然科学基金(10978019)

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引力透镜类星体SDSS J1004+4112的吸收线研究
2020年
基于SDSS (Sloan Digital Sky Survey,斯隆数字巡天) DR15 (The Data Release 15,第15期数据)的光谱,分析引力透镜类星体SDSS J1004+4112两个像(A和B像之间的角距离约为3.73′′)的光谱。通过C IVλλ1548?, 1551?和Mg Ⅱλλ2796?, 2803?吸收双线,在A、B两个像的光谱上证认得到两个C IV吸收线系统和两个Mg Ⅱ吸收线系统。在引力透镜类星体SDSS J1004+4112 A, B两个像的光谱上C Ⅳ吸收线系统没有明显的差异(吸收线等值宽度差异的置信水平N△W<3),吸收体在视线方向上的横向尺度Dtra≈127.5 pc,相对类星体的速度βs<0.06,两视线上的吸收体可能是来源于类星体同一区域的本征吸收体。但是,两个Mg Ⅱ吸收线系统在两个像光谱上存在明显的差异(N△W> 3);A像光谱上只存在红移为0.831 1±0.000 3的Mg Ⅱ吸收线系统,吸收体的Dtra≈21.319 kpc;而B像光谱上只存在系统红移为0.671 1±0.006 1的Mg Ⅱ吸收线,吸收体的Dtra≈26.280 kpc。
黄红艳谢照华彭瑞杜雷鸣谭灿刘小鹏顾敏峰
关键词:吸收线证认光谱
The correlation between the Doppler factor and broad line region luminosity in blazars被引量:1
2012年
The disk-jet symbiosis is a fundamental problem in our understanding of the Active Galactic Nuclei(AGN).We explore the relation between the Doppler factors of the jet of blazars and their broad line region luminosity LBLR.Since different methods measuring might differ substantially,we use data obtained from 3 independent methods and compile 3 samples of sources for each of them,respectively.Two samples consist of blazars,that is,Flat Spectrum Radio Quasars(FSRQs) and BL Lacertae objects(BL Lacs),and the other consists of BL Lacs.is one of the most important jet properties and LBLR is thought to be the proxy of the accretion power.Correlation analysis to these samples shows that there exists a significant correlation between and LBLR,which supports the idea that the jet powering process is closely linked with the accretion process and provides new evidence for disk-jet connection.Furthermore,the results are consistent with the idea that the Blandford-Znajek mechanism is sufficient for BL Lacs and a hybrid model is needed for FSRQs.
DU LeiMingBAI JinMing
关键词:耀变体活动星系核
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