论文标题
NLR大小的依赖性对低红移AGN的[OIII]光度，并具有双峰宽Balmer发射线
Dependence of NLRs sizes on [OIII] luminosity in low redshift AGN with double-peaked broad Balmer emission lines
论文作者
论文摘要
在手稿中，报道了一个简单而有趣的结果，该结果是关于38个低红移（$ z <0.1 $）AGN的NLRS大小的上限，具有双峰宽发射线（双峰膨胀的斑点），以便检查NLRS尺寸在1型AGN和2型Agn obe之间和类似的empuical empure empurical empure condence nlrs大小是否umin umin上。为了纠正对1型AGN投影的NLR大小的倾斜作用，通常将积聚磁盘起源用于描述38个双峰式爆炸的中央磁盘样BLR的确定倾斜度的双峰宽H $α$。然后，考虑到固定的SDSS纤维半径，可以估计38个双峰式播放的NLRS大小的上限。同时，使用连续亮度与\ o3〜光度之间的强线性相关性，以确认38个双峰盖的\ o3〜排放完全覆盖在SDSS纤维中。考虑到经过重新校正后的测量\ O3〜光泽度，38个双峰式播放的NLRS大小的上限在99.9999 \％的置信区间内NLRS大小之间的经验关系和\ o3〜Ulinosie type-2 AGN类型的\ o3〜亮度的预期结果的结果。在当前阶段，没有线索可以通过NLR的空间属性来挑战AGN的统一模型。
In the manuscript, the simple but interesting results are reported on the upper limits of NLRs sizes of a small sample of 38 low redshift ($z<0.1$) AGN with double-peaked broad emission lines (double-peaked BLAGN), in order to check whether the NLRs sizes in type-1 AGN and type-2 AGN obey the similar empirical dependence on \o3~ luminosity. In order to correct the inclination effects on projected NLRs sizes of type-1 AGN, the accretion disk origin is commonly applied to describe the double-peaked broad H$α$ leading to the determined inclination angles of central disk-like BLRs of the 38 double-peaked BLAGN. Then, considering the fixed SDSS fiber radius, the upper limits of NLRs sizes of the 38 double-peaked BLAGN can be estimated. Meanwhile, the strong linear correlation between continuum luminosity and \o3~ luminosity is applied to confirm that the \o3~ emissions of the 38 double-peaked BLAGN are totally covered in the SDSS fibers. Considering the reddening corrected measured \o3~ luminosity, the upper limits of NLRs sizes of the 38 double-peaked BLAGN are within the 99.9999\% confidence interval of the expected results from the empirical relation between NLRs sizes and \o3~ luminosity in the type-2 AGN. In the current stage, there are no clues to challenge the Unified model of AGN, through the space properties of NLRs.
