NAOC Open IR  > 空间科学研究部
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
2003
Source PublicationHIGH ENERGY PROCESSES AND PHENOMENA IN ASTROPHYSICS
Issue214Pages:273-274
AbstractWe 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.
Indexed ByISTP ; SCI
Language英语
WOS IDWOS:000189431800044
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8440
Collection空间科学研究部
Affiliation1.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
Recommended Citation
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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