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Emission line properties of seyfert 1 type AGN from RASS
Xu, DW; Komossa, S; Wei, JY; Zheng, XZ; Qian, Y; Li, XD; Trimble, V; Wang, ZR
刊名HIGH ENERGY PROCESSES AND PHENOMENA IN ASTROPHYSICS
2003
期号214页码:273-274
英文摘要We present the optical emission line properties of a sample of 155 bright X-ray selected ROSAT Seyfert 1 type AGN. The measured properties are gathered for correlation analysis. The strong correlations between Hbeta redshift, flux ratios of Fe II to Hbeta broad component and [O III] to Hbeta narrow component are found.
收录类别ISTP ; SCI
语种英语
WOS记录号WOS:000189431800044
内容类型期刊论文
源URL[http://ir.bao.ac.cn/handle/114a11/8440]  
专题国家天文台_空间科学研究部
作者单位1.Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
2.Natl Astron Observ, Beijing 100012, Peoples R China
3.Tsing Hua Univ, Beijing 100080, Peoples R China
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GB/T 7714
Xu, DW,Komossa, S,Wei, JY,et al. Emission line properties of seyfert 1 type AGN from RASS[J]. HIGH ENERGY PROCESSES AND PHENOMENA IN ASTROPHYSICS,2003(214):273-274.
APA Xu, DW.,Komossa, S.,Wei, JY.,Zheng, XZ.,Qian, Y.,...&Wang, ZR.(2003).Emission line properties of seyfert 1 type AGN from RASS.HIGH ENERGY PROCESSES AND PHENOMENA IN ASTROPHYSICS(214),273-274.
MLA Xu, DW,et al."Emission line properties of seyfert 1 type AGN from RASS".HIGH ENERGY PROCESSES AND PHENOMENA IN ASTROPHYSICS .214(2003):273-274.
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