论文标题
BH质量，喷气和积聚磁盘连接：无线电和射电Quiet类星体的分析
BH Mass, Jet and Accretion Disk Connection: An Analysis of Radio-loud and Radio-quiet Quasars
论文作者
论文摘要
调查显示了无线电（RL）类星体构成$ 10 \％$ - $ 15 \％$ $ 15 \％$的总人口。但是，未知是否在不同的参数空间之间保持无线电大量分数（RL类星体/总类型）仍然一致。这项研究表明，H $β$和MGII宽发射线的全宽度最大速度（FWHM）速度增加了无线电大分的增加。我们的数据已从Shen等人获得。 （2011）目录。为了研究原因，在这项初步研究中，我们分析了各种特性，例如隆期亮度，光学连续性光度，黑洞（BH）质量（BH）质量和RL类星体的增生速率和RQ Quasars样品，其FWHM大于15000 km/s（高宽线）。从分布中，我们可以得出所有高宽线中所有属性的结论，RL类星体的值高于RQ类星体。我们已经预测RL类星体本质上比RQ类星体更明亮，并且还可以从我们的结果中预测BH质量喷射连接和积聚磁盘的连接，但要得出结论，需要进行任何更多分析。
Surveys have shown radio-loud (RL) quasars constitute $10 \%$-$15 \%$ of the total quasar population. However, it is unknown if the radio-loud fraction (RL quasars/Total quasars) remains consistent among different parameter spaces. This study shows that radio-loud fraction increases for increasing full width half maximum (FWHM) velocity of the H$β$ and MgII broad emission line. Our data has been obtained from Shen et al. (2011) catalogue. To investigate the reason, in this preliminary study we analyse various properties like bolometric luminosity, optical continuum luminosity, black hole (BH) mass and accretion rate of RL quasars and RQ quasars sample which have FWHM greater than 15000km/s (High broad line). From the distributions we can conclude for all the properties in high broad line, RL quasars are having higher values than RQ quasars. We have predicted RL quasars are intrinsically brighter than RQ quasars and also predicted BH mass-jet connection and accretion disk-jet connection from our results but to conclude anything more analysis is needed.
