The prevalence of narrow optical Fe II emission lines in type 1 active galactic nuclei

Astrophysical Journal Letters

Volumn 721, Issue 2 PART 2, 2010, Pages

  Dong, Xiao Bo ^a,b   Ho, Luis C ^b   Wang, Jian Guo ^a,c,d   Wang, Ting Gui ^a   Wang, Huiyuan ^a   Fan, Xiaohui ^e   Zhou, Hongyan ^a  

^a UNIVERSITY OF SCIENCE AND TECHNOLOGY OF CHINA   (China)

^b CARNEGIE OBSERVATORIES   (United States)

^c CHINESE ACADEMY OF SCIENCES   (China)

^d UNIVERSITY OF CHINESE ACADEMY OF SCIENCES   (China)

^e UNIVERSITY OF ARIZONA   (United States)

Author keywords

Accretion, accretion disks; Galaxies: active; Line: formation; Line: identification; Quasars: emission lines; Radiation mechanisms: general

Indexed keywords

EID: 78649269872     PISSN: 20418205     EISSN: 20418213     Source Type: Journal    
DOI: 10.1088/2041-8205/721/2/L143     Document Type: Article

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