CASIA OpenIR  > 模式识别国家重点实验室  > 机器人视觉
Emission lines properties of the radio-loud quasar LAMOST J1131+3114 (Research Note)
Shi, Z. X.1,2,3; Comte, G.2,4; Luo, A. L.2; Zhao, Y. H.2; Zhao, J. K.2,5; Oswalt, T. D.5; Wu, F. C.1
发表期刊ASTRONOMY & ASTROPHYSICS
2014-04-01
卷号564
文章类型Article
摘要The radio-loud quasar LAMOST J1131+3114 (Ton 580, B2 1128+315), showing asymmetrical profile in H beta and [OIII] lines, has been selected from the LAMOST Pilot Survey for further study. We present an analysis of its emission lines by means of multiple Gaussian fitting, performed on LAMOST, Apache Point Observatory, and archival spectra. The broad line region, with an H beta line of FWHM similar to 4000 km s(-1) has been fit with a double Gaussian, one of which is very broad and redshifted from the reference frame. The object is a likely Population B quasar. The [OIII] lambda lambda 4959,5007 lines profiles of the source have been formally fit with two Gaussian components, one of which is as broad as similar to 700 km s(-1). This broader component, if physically meaningful, appears to be subject to moderate velocity shock excitation. The forbidden line ratios correspond to a poorly populated area in standard diagnostic diagrams of AGN narrow line regions.
关键词Quasars: Individual: Lamost j1131+3114 Quasars: Emission Lines Galaxies: Jets Galaxies: Interactions Galaxies: Kinematics And Dynamics
WOS标题词Science & Technology ; Physical Sciences
关键词[WOS]ACTIVE GALACTIC NUCLEI ; BLACK-HOLE MASS ; DIGITAL SKY SURVEY ; X-RAY ; STELLAR OBJECTS ; OPTICAL VARIABILITY ; EDDINGTON RATIO ; LUMINOSITY ; SPECTRA ; REGION
收录类别SCI
语种英语
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
WOS记录号WOS:000334671000089
引用统计
被引频次:6[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ia.ac.cn/handle/173211/2972
专题模式识别国家重点实验室_机器人视觉
作者单位1.Chinese Acad Sci, Inst Automat, Natl Lab Pattern Recognit, Beijing 100190, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China
3.Univ Chinese Acad, Beijing 100049, Peoples R China
4.Aix Marseille Univ, CNRS, Inst Pytheas, LAM,UMR 7326, F-13388 Marseille, France
5.Florida Inst Technol, Phys & Space Sci Dept, Melbourne, FL 32901 USA
第一作者单位模式识别国家重点实验室
推荐引用方式
GB/T 7714
Shi, Z. X.,Comte, G.,Luo, A. L.,et al. Emission lines properties of the radio-loud quasar LAMOST J1131+3114 (Research Note)[J]. ASTRONOMY & ASTROPHYSICS,2014,564.
APA Shi, Z. X..,Comte, G..,Luo, A. L..,Zhao, Y. H..,Zhao, J. K..,...&Wu, F. C..(2014).Emission lines properties of the radio-loud quasar LAMOST J1131+3114 (Research Note).ASTRONOMY & ASTROPHYSICS,564.
MLA Shi, Z. X.,et al."Emission lines properties of the radio-loud quasar LAMOST J1131+3114 (Research Note)".ASTRONOMY & ASTROPHYSICS 564(2014).
条目包含的文件
条目无相关文件。
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Shi, Z. X.]的文章
[Comte, G.]的文章
[Luo, A. L.]的文章
百度学术
百度学术中相似的文章
[Shi, Z. X.]的文章
[Comte, G.]的文章
[Luo, A. L.]的文章
必应学术
必应学术中相似的文章
[Shi, Z. X.]的文章
[Comte, G.]的文章
[Luo, A. L.]的文章
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。