SDSS J1042-0018:a Broad Line AGN but Misclassified as an HⅡGalaxy in the BPT Diagram by Flux Ratios of Narrow Emission Lines  

作　　者：Yi Cao Si-Dan Zhao Xing-Yu Zhu Hai-Chao Yu Yi-Wei Wang Xue-Guang Zhang 

机构地区：[1]School of Physics and Technology,Nanjing Normal University,Nanjing 210023,China

出　　处：《Research in Astronomy and Astrophysics》2022年第4期114-122,共9页天文和天体物理学研究（英文版）

基　　金：the kind support of Starting Research Fund of Nanjing Normal University;the kind support of NSFC-12173020;the kind support of Da Chuang project of Nanjing Normal University for undergraduate students。

摘　　要：In this paper,we discuss properties of SDSS J1042-0018 which is a broad line active galactic nucleus(AGN)but misclassified as an H II galaxy in the BPT diagram(SDSS J1042-0018 is called a misclassified broad line AGN).The emission lines around Hαand around Hβare well described by different model functions,considering broad Balmer lines to be described by Gaussian or Lorentz functions.Different model functions lead to different determined narrow emission line fiuxes,but the different narrow emission line fiux ratios lead SDSS J1042-0018 as an H II galaxy in the BPT diagram.In order to explain the unique properties of the misclassified broad line AGN SDSS J1042-0018,two methods are proposed,the star-forming contributions and the compressed narrow emission line regions with high electron densities near to critical densities of forbidden emission lines.Fortunately,the strong star-forming contributions can be preferred in SDSS J1042-0018.The misclassified broad line AGN SDSS J1042-0018,well explained by star-forming contributions,could provide further clues on the applications of BPT diagrams to the normal broad line AGNs.

关 键 词：active galaxies active galactic nuclei emission line galaxies QUASARS 

分 类 号：P157.6[天文地球—天文学]